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%Description        Aladin sky atlas (ASU parameters).
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%Url                https://aladin.cds.unistra.fr/AladinLite/app/?survey=$1&zoom=$2&target=$3&width=$4&height=$5
%Param.Description  $1= Survey identifier (e.g: P/DSS2/red)
%Param.Description  $2= Zoom value in degrees
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%Param.Description  $5= Height of Aladin Lite

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%ActionName         AladinPoolServlet
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%Test               param="get aladin M101;grid on"

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%Param.Description  $3=Language (us|fr)
%Param.DataType     $1=CDS'simbad'I
%Param.DataType     $1=Coo(J2000,COO)
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%P.0                2 3

%ActionName         AladinSaturationTest
%Description        Test de saturation de la RAM et du disque de la machine aladix (serveur\nimages Bonnarel)
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%Test               noparam pattern="Ca roule"

%ActionName         AladinX.help
%Description        On line documentation for Aladin Xwindows
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%Url                http://aladin.cds.unistra.fr/intro.html
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%ActionName         AlaskyGlobal
%Description        Test de fonctionnement d'alasky ou alaskybis
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%Test               param="1997ApJS..111...73K" pattern="a traditional particle-mesh technique"
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%ActionName         AstroCoo.WS
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%Owner              CDS'ws
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%Url                http://cdsws.u-strasbg.fr/axis/services/AstroCoo?$1
%Test               param="wsdl" pattern="convertResponse2"
%ResultDataType     soap
%Doc.Technical      http://cds.unistra.fr/cdsws/astroCoo.gml

%ActionName         AstroGrid.home
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%DefaultAnchorText  AstroGrid

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%Param.Description  $1=Last name of Astronomy person
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%Url                http://cds.unistra.fr/astroweb.html
%DefaultAnchorText  <B>A</B>stroWeb
%FullTextResult     <A HREF="$url" target="_top">$text</A>
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%DefaultAnchorText  <B>A</B>stroWeb NRAO
%Test               param="AstroWeb"
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%DefaultAnchorText  <B>A</B>stroWeb Cambridge
%Test               param="AstroWeb"
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%ActionName         AstroWebSearch
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%VersionNumber      1641202928  2022/01/03 11:42:08
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%Param.Description  $1=Wais query
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%Test               param="telescope"
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%ActionName         Atom
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%Owner              CDS'VizieR
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%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.chemistry-reference.com/pdictable/q_elements.asp?Symbol=$1
%Param.DataType     $1=misc'query/keywords
%Test               param="Hg"
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%Id                 B/simbad
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%Test.Result        0  2023/05/26 16:16:01
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%Url                http://aladin.cds.unistra.fr/java/Bookmarks-v10.ajs
%Aladin.Bookmarks   DSS,PanSTARRS,SDSS,2MASS,GALEX,Gaia,Simbad,NED
%Aladin.Profile     >9

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%Url                http://aladin.cds.unistra.fr/java/Bookmarks-v8.ajs
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%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/AllWISE/WISE-cube
%VerboseDescr       All WISE cube (W1,W2,W3,W4) from raw Atlas Images.\nResampled in HEALPix by Thomas Boch [CDS]
%Copyright          WISE acknowledgment
%Acknowledgement    This Progressive Survey distribution makes use of data products from the Wide-field Infrared Survey Explorer,\nwhich is a joint project of the University of California, Los Angeles,\nand the Jet Propulsion Laboratory/California Institute of Technology, and NEOWISE,\nwhich is a project of the Jet Propulsion Laboratory/California Institute of Technology.\nWISE and NEOWISE are funded by the National Aeronautics and Space Administration.
%Copyright.url      http://wise2.ipac.caltech.edu/docs/release/allwise/expsup/sec1_6b.html
%Id                 C/AllWISE
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%Aladin.HpxParam    8 jpeg fits cube

%ActionName         C-B0DEGA.hpx
%Description        B0DEGA: Below 0 DEgree GAlaxies
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%VersionNumber      1465811895  2016/06/13 11:58:15
%Url                http://amiga.iaa.es/HiPS/3DCollections/B0DEGA
%VerboseDescr       The SMA B0DEGA (Below 0 DEgree GAlaxies) project, a high resolution (3 arcsec) survey of CO(2-1) (and isotopes) emission of the circumnuclear regions (1 arcmin) of 30 previously unexplored southern nearby galaxies obtained using the Submillimeter Array (SMA). The sample is composed of IR-bright galaxies (2.58 x S60 + S100 > 31.5 Jy) with recession velocities V < 7000 km/s.
%Copyright          AMIGA Group, IAA-CSIC, Spain
%Origin             svo.amiga.iaa.es
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%Copyright.Url      http://b0dega.iaa.es/
%SkyFraction        2.344E-6
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%Aladin.HpxParam    11 cube equatorial png fits
%Aladin.Date        2015-06-09T09:04Z

%ActionName         C-CALIFA-V500-DR2.hpx
%Description        CALIFA DR2 V500 (R~850, 3750-7500 A)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CALIFA/V500DR2
%VerboseDescr       The Calar Alto Legacy Integral Field Area survey is one of the largest IFS surveys performed to date. At its completion it will comprise 600 galaxies, observed with the PMAS spectrograph in the PPAK mode, covering the full spatial extent of these galaxies up to two effective radii. The wavelength range between 3700 and 7500 is sampled with two spectroscopic configurations, a high resolution mode (V1200, R~1700, 3700-4200), and a low resolution mode (V500, R~850, 3750-7500). A detailed explanation of the survey is given in the CALIFA Presentation Article (Sanchez et al. 2012). The second CALIFA Data Release (DR2) provides to the public the fully reduced and quality control tested datacubes of 200 objects in both setups (V500 and V1200). Each datacube contains ~1000 independent spectra, thus in total this DR comprises ~400,000 total independent spectra (~1.5 millon after cube reconstruction). The details of the data included in this DR are described in the CALIFA DR2 Article (Garcia Benito et al. 2014). The differences in the data reduction pipeline adopted for this dataset are described in this article too, in comparison with the current solution adopted for DR1 (Husemann et al. 2013)
%Copyright          Based on observations collected at the Centro Astronomico Hispano Aleman (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut fur Astronomie and the Instituto de Astrofisica de Andalucia (CSIC)
%Origin             CDS
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%Copyright.Url      http://www.caha.es/CALIFA/public_html/?q=content/califa-2nd-data-release
%SkyFraction        2.937E-4
%Aladin.XLabel      The Calar Alto Legacy Integral Field Area survey - V500 resolution mode (CALIFA V500) DR2
%Aladin.Tree        Cube
%Aladin.HpxParam    9 cube equatorial png
%Aladin.Date        2016-06-03T09:56Z

%ActionName         C-CGPS-HI.hpx
%Description        CGPS data cubes HI (21cm)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CGPS/
%VerboseDescr       The Dominion Radio Astrophysical Observatory, in collaboration with an international Consortium of astronomers, has carried out a high-resolution survey of the atomic hydrogen and radio continuum emission from our Milky Way galaxy. The observations of 373 fields with the DRAO Synthesis Telescope are presented in sixty-eight 5 deg x 5 deg mosaics, covering Galactic longitudes from L = 63 to 175 degrees and latitudes from B = -3.5 to +5.5 degrees and a latitude extension to B = +17.5 degrees between L = 100 to 116.5 degrees, with a resolution as small as 1 arcminute. For each mosaic (1024 x 1024 pixels), atomic hydrogen observations are presented as a data "cube" with 272 spectral channels having a velocity resolution of 1.3 km/s. Stokes I continuum images at 1420 MHz and 408 MHz are produced, as well as selected Stokes Q, U and V images at 1420 MHz. Complementary images in the four IRAS infrared bands and data cubes of CO (J=1-0) emission have also been created as part of the Survey.
%Copyright          The following materials are copyrighted by the Canadian Galactic Plane Survey/Releve Canadien du Plan Galactique (CGPS/RCPG). They are intended as a news release material and for use for educational, academic, and research purposes and are not intended for commercial sale. Please contact Jayanne English (email: jayanne_english@umanitoba.ca) to inquire about permission for other non-commercial and/or commercial uses
%Origin             CDS
%Id                 C/CGPS-HI
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ras.ucalgary.ca/CGPS/
%SkyFraction        0.03684
%Aladin.XLabel      Canadian Galactic Plane Survey data cubes HI (21cm)
%Aladin.Tree        Cube
%Aladin.HpxParam    5 cube equatorial png fits
%Aladin.Date        2015-06-05T12:31Z

%ActionName         C-EGRET-Dif-Cube.hpx
%Description        Diffuse Gamma-ray EGRET map cube - 30-10000MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_Cube
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 30 MeV to 10000MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory.
%Copyright          See ApJ Volume 621, March 2005
%Id                 C/EGRET/Dif
%Origin             CDS
%Aladin.XLabel      EGRET Dif Cube
%Aladin.Tree        Cube/Test
%Aladin.Profile     >=8.040 beta
%Aladin.HpxParam    3 jpeg fits cube equ
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html

%ActionName         C-GALFAHI-Narrow.hpx
%Description        GALFA-HI Narrow
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GALFAHI/GALFAHI-Narrow/
%VerboseDescr       Data Release 1 (DR1) of the GALFA HI data set, obtained with the Arecibo L-band Feed Array (ALFA) on the Arecibo 305m telescope. This neutral hydrogen survey has a resolution of ~4', a spectral resolution of 0.18km/s for velocities -190 km/s<V<190 km/s. Details on the observations and this release are in Peek et al. 2011.
%Copyright          GALFA-HI Data Archive
%Origin             CDS
%Id                 C/GALFAHI/Narrow
%Aladin.Profile     >6.1
%Copyright.Url      https://purcell.ssl.berkeley.edu
%SkyFraction        0.3164
%Aladin.XLabel      GALFA-HI Narrow
%Aladin.Tree        Cube
%Aladin.HpxParam    3 cube equatorial png fits
%Aladin.Date        2016-12-20T09:52Z

%ActionName         C-HI4PI-HI.hpx
%Description        HI4PI HI survey (individual cubes)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HI4PI/C_HI4PI_NHI
%VerboseDescr       The HI4PI data release comprises 21-cm neutral atomic hydrogen data of the Milky Way (-600km/s<vlsr<+600km/s for declination >0deg; -470km/s<vlsr<+470km/s for declination <0deg) as observed with the 100-m radio telescope at Effelsberg and the 64-m radio telescope at Parkes. HI4PI covers the full 4-pi sky.
%Copyright          VizieR Service, CDS (ftp : J/A+A/594/A116/)
%Origin             CDS
%Id                 C/HI4PI/HI
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      HI4PI HI
%Aladin.Tree        Cube
%Aladin.HpxParam    3 cube equatorial jpeg fits
%Aladin.Date        2017-06-27T16:37Z

%ActionName         C-HIPASS.hpx
%Description        HIPASS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HIPASS
%VerboseDescr       The `HI Parkes All Sky Survey' (HIPASS) covers the whole southern sky as well as northern declinations up to +25 degrees. HIPASS commenced in Feb 1997, and the last northern scans were taken in 2002. HIPASS was carried out with the Australia Telescope National Facility's Parkes telescope Parkes 64-m telescope equipped with a novel 21-cm multibeam system. The latter comprises a cooled, 13 beam receiver and digital correlator (Staveley-Smith et al. 1996, Wilson et al. 1997 and Sinclair et al. 1997). The 64 MHz observing band, centred on 1394.5 MHz, was divided into 1024 channels, providing a velocity range of -1280 < cz < 12700 km/s with a channel width of approx. 13.2 km/s and a velocity resolution of 18 km/s. The HIPASS integration time per beam is 450s. After gridding an r.m.s. noise of about 13.3 mJy was achieved in the first set of HIPASS cubes. The observations and techniques used to calibrate and image the data are described in Barnes et al. (2001). The processing algorithms are successfully designed to be statistically robust to the presence of interference signals and are particular to imaging point (or nearly point) sources, not extended emission. Specifically, a major improvement in image quality is obtained by designing a median-gridding algorithm which uses the median estimator in place of the mean estimator. While the average Parkes beam FWHM is 14.3 arcmin, the average gridded HIPASS beam is about 15.5 arcmin. The full data release contains data from 538 data cubes (size: 8o x 8o, 388 over the entire southern sky (DEC < +2o), and 150 over the northern sky, (DEC < +25o). The one-dimensional spectral data for a given position is available for downloading in a variety of different formats.
%Copyright          Creative Commons Attribution 4.0 International Licence: Koribalski, Baerbel; Staveley-Smith, Lister (2004): The HI Parkes All Sky Survey (HIPASS) image cubes. v1. CSIRO. Data Collection. 102.100.100/70188 https://doi.org/10.25919/5c36de6d37141
%Origin             CDS
%Id                 C/HIPASS
%Aladin.Profile     >6.1
%Copyright.Url      https://data.csiro.au/dap/landingpage?pid=csiro:32333
%SkyFraction        0.7188
%Aladin.XLabel      HIPASS
%Aladin.Tree        Cube
%Aladin.HpxParam    0 cube equatorial png fits
%Aladin.Date        2019-01-18T22:14Z

%ActionName         C-HST-GOODS.hpx
%Description        HST ACS GOODS composite cube (b,v,i & z bands)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/GOODS/GOODS-cube
%VerboseDescr       The C/HST/GOODS Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in b,v,i and z bands as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities,\nto survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Id                 C/HST/GOODS
%Origin             CDS
%Acknowledgement    All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555.""
%Copyright.url      http://www.stsci.edu/institute/Copyright
%Aladin.XLabel      GOODS cube
%Aladin.Tree        Cube/Test
%Aladin.Profile     >=8.040 beta
%Aladin.HpxParam    14 png fits cube
%Aladin.Date        2014-04-15T12:00Z

%ActionName         C-HST.hpx
%Description        HST observations (->1/6/2013) provided as a composite cube
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/HST/HST-cube
%VerboseDescr       The HST cube Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations between the beginning of the mission  to the 1st of June 2013.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.
%Copyright          from CADC
%Id                 C/HST
%Origin             CDS
%Acknowledgement    All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency. ""
%Copyright.url      http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/hst/
%Aladin.XLabel      HST cube
%Aladin.Tree        Cube/Test
%Aladin.Profile     >=8.040 beta
%Aladin.HpxParam    14 png fits cube

%ActionName         C-IRIS.hpx
%Description        IRAS composite cube
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/C-IRAS
%Id                 C/IRAS
%Origin             CDS
%Aladin.XLabel      IRIS cube
%Aladin.Tree        Cube/Test
%Aladin.Profile     >=8.040 beta
%Aladin.HpxParam    3 jpeg fits galactic cube

%ActionName         C-MUSE-M42.hpx
%Description        MUSE map of the central Orion Nebula (M 42)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/MUSE/MUSE-M42
%VerboseDescr       Integral-field spectroscopic dataset of the central part of the Orion Nebula (M 42), observed with the MUSE instrument at the ESO VLT (reduced the data with the public MUSE pipeline) representing a FITS cube with a spatial size of ~5.9'x4.9' (corresponding to ~0.76 pc x 0.63 pc) and a contiguous wavelength coverage of 4595...9366 Angstrom, spatially sampled at 0.2", with a sampling of 1.25 Angstrom in dispersion direction.
%Copyright          Copyright mention of the original data
%Origin             CDS
%Id                 C/MUSE-M42
%Aladin.Profile     >6.1 beta
%Copyright.Url      http://muse-vlt.eu/science/m42/
%SkyFraction        2.980E-7
%Aladin.XLabel      MUSE-M42
%Aladin.Tree        Cube
%Aladin.HpxParam    12 cube equatorial png fits
%Aladin.Date        2015-07-07T00:29Z

%ActionName         C-Mopra-12CO.hpx
%Description        Mopra 12CO
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Mopra/12CO/hips_12CO
%VerboseDescr       This product was build only with Mopra cubes having the same velocity axis. The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370°. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300?350° and latitudes |b| ? 0.5°. These data have been taken at 0.6arcminute spatial resolution and 0.1kms?1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109?115 GHz J = 1?0 transitions of 12CO, 13CO, C18O and C17O.
%Copyright          MOPRA
%Origin             CDS
%Id                 C/Mopra/12CO
%Aladin.Profile     >6.1
%SkyFraction        6.148E-4
%Aladin.XLabel      Mopra 12CO
%Aladin.Tree        Cube
%Aladin.HpxParam    4 cube equatorial png fits
%Aladin.Date        2019-03-04T17:37Z

%ActionName         C-Mopra-13CO.hpx
%Description        Mopra 13CO
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Mopra/13CO/hips_13CO
%VerboseDescr       This product was build only with Mopra cubes having the same velocity axis. The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370°. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300?350° and latitudes |b| ? 0.5°. These data have been taken at 0.6arcminute spatial resolution and 0.1kms?1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109?115 GHz J = 1?0 transitions of 12CO, 13CO, C18O and C17O.
%Copyright          MOPRA
%Origin             CDS
%Id                 C/Mopra/13CO
%Aladin.Profile     >6.1
%SkyFraction        5.540E-4
%Aladin.XLabel      Mopra 13CO
%Aladin.Tree        Cube
%Aladin.HpxParam    4 cube equatorial png fits
%Aladin.Date        2019-03-05T14:38Z

%ActionName         C-Mopra-C17O.hpx
%Description        Mopra C17O
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Mopra/C17O/hips_C17O
%VerboseDescr       This product was build only with Mopra cubes having the same veloicty axis. The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370°. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300?350° and latitudes |b| ? 0.5°. These data have been taken at 0.6arcminute spatial resolution and 0.1kms?1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109?115 GHz J = 1?0 transitions of 12CO, 13CO, C18O and C17O.
%Copyright          MOPRA
%Origin             CDS
%Id                 C/Mopra/C17O
%Aladin.Profile     >6.1
%SkyFraction        5.928E-4
%Aladin.XLabel      Mopra C17O
%Aladin.Tree        Cube
%Aladin.HpxParam    4 cube equatorial png fits
%Aladin.Date        2019-03-06T10:39Z

%ActionName         C-Mopra-C18O.hpx
%Description        Mopra C18O
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Mopra/C18O/hips_C18O
%VerboseDescr       This product was build only with Mopra cubes having the same velocity axis. The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370°. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300?350° and latitudes |b| ? 0.5°. These data have been taken at 0.6arcminute spatial resolution and 0.1kms?1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109?115 GHz J = 1?0 transitions of 12CO, 13CO, C18O and C17O.
%Copyright          MOPRA
%Origin             CDS
%Id                 C/Mopra/C18O
%Aladin.Profile     >6.1
%SkyFraction        3.681E-4
%Aladin.XLabel      Mopra C18O
%Aladin.Tree        Cube
%Aladin.HpxParam    4 cube equatorial png fits
%Aladin.Date        2019-03-06T09:42Z

%ActionName         C-SimbadHeatmaps.hpx
%Description        Simbad Composite cube built from Simbad literature object citations
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/SimbadHeatmaps/time-cube
%Id                 C/SimbadHeatmaps
%Origin             CDS
%Aladin.XLabel      Simbad Heatmaps cube
%Aladin.Tree        Cube/Test
%Aladin.Profile     >=8.040 beta
%Aladin.HpxParam    3 jpeg fits cube

%ActionName         C-WHISP-sample.hpx
%Description        AMIGA galaxies in the WHISP (Westerbork HI Survey of Irregular and SPiral galaxies) Survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1465811895  2016/06/13 11:58:15
%Url                http://amiga.iaa.es/HiPS/3DCollections/WHISP
%VerboseDescr       This is a subsample of 27 radiointerfermetric datacubes of the larger WHISP database. These 27 galaxies are part of the AMIGA catalog of isolated galaxies, where WHISP is a survey of the neutral hydrogen component in spiral and irregular galaxies with the Westerbork Synthesis Radio Telescope (WSRT).
%Copyright          Westerbork Synthesis Radio Telescope
%Origin             svo.amiga.iaa.es
%Id                 C/WHISP-sample
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astron.nl/wow/testcode.php?project=3
%SkyFraction        0.004272
%Aladin.XLabel      WHISP-sample
%Aladin.Tree        Cube
%Aladin.HpxParam    6 cube equatorial png fits
%Aladin.Date        2015-06-09T09:04Z

%ActionName         C-WMAP-cube-9yr.hpx
%Description        WMAP cube - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/WMAP9yr/WMAPCube9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The WMAP cube is built from the 5 original bands (K/23GHz, Ka/33GHz, Q/41GHz, V/61GHz, W/94GHz)
%Copyright          from CDS (original data from LAMBDA)
%Id                 C/WMAP/cube/9yr
%Origin             CDS
%Aladin.Profile     >6.1 beta
%Aladin.Tree        Cube/Test
%Copyright.url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%Aladin.XLabel      WMAP Cube 9yr
%Aladin.HpxParam    3 png jpeg fits cube
%Aladin.MenuNumber  ZZZ

%ActionName         CADC
%Description        Canadian Astronomical Data Center (CADC)
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/sia/query?POS=$1,$2&SIZE=$3&FORMAT=image/fits&VERB=2
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.Value        $3=0.17
%ResultDataType     Mime(sia/xml)
%VerboseDescr       The Canadian Virtual Observatory (CVO) provides this SIA server access for some CADC archives (decompose mosaic images into single extension FITS files , cutout of the region-of-interest when it is smaller than the image, WCS correction of returned FITS files.
%VerboseDescr       The Canadian Virtual Observatory (CVO) provides this SIA server access for some CADC archives (decompose mosaic images into single extension FITS files , cutout of the region-of-interest when it is smaller than the image, WCS correction of returned FITS files.
%Doc.User           http://www.cadc.hia.nrc.gc.ca/cadc/
%Aladin.Menu        Archives...
%Aladin.Label       Canadian Astronomical Data Center (CADC)
%Aladin.LabelPlane  $4 $1
%Aladin.Logo        CADCLogo.gif

%ActionName         CAI
%Description        VO-Paris Southern Atlas (VOPSAT)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1507560157  2017/10/09 16:42:37
%Url                http://voparis-srv.obspm.fr/sia/sia_mama.php?survey=$4&POS=$1,$2&SIZE=$3&FORMAT=image/fits
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.Description  $4=Survey
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.Value        $3=0.17
%Param.Value        $4=All - All surveys
%Param.Value        $4=ESOR - ESO survey / R color
%Param.Value        $4=SRCJ - SERC survey / J color
%Param.Value        $4=POSSE - POSS survey / E color
%ResultDataType     Mime(sia/xml)
%VerboseDescr       This is the first step in a VO-compliant  publication of Schmidt surveys of the southern sky digitized with the MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI). The pixel size is 10 micrometers (0.7 arc-sec). The ESO-R atlas will be followed by the SRC-J and the southern part of the POSS1_E atlases. Catalogs of the detected objects will also be available. The bandpass is : close to R (combination: IIIaF + RG 630)
%Institute          VO-Paris
%Doc.User           http://vo.obspm.fr/sia/eso-r.html
%Aladin.Label       VO-Paris MAMA Atlas
%Aladin.Menu        Others...
%Aladin.LabelPlane  CAI $4 $1
%Aladin.Profile     <10

%ActionName         CASSIS
%Description        CASSIS interactive spectrum analyser (plugin version)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1665996628  2022/10/17 10:50:28
%VerboseDescr       The CASSIS (Centre d'Analyse Scientifique de Spectres Instrumentaux et Synthéques) software has been developed by CESR/IRAP since 2005. CASSIS uses the SSAP (Single Spectral Access Protocol) and EPN-TAP (EuroPlaNet Table Access Protocol) protocols to access the IVOA services in order to retrieve any spectra (Hubble, Corot, Splatalogue, ISO, etc; the complete list dans be found at http://registry.euro-vo.org webpage) via our SSAP or EPN-TAP module. You can also process to line identification using the VAMDC (Virtual And Molecular Database Center) or SLAP (Simple Line Access Protocol) protocols. Of course, CASSIS uses the SAMP messaging protocol (Simple Application Messaging Protocol) that enables astronomy software tools to interoperate and communicate.
%Institute          Institut de Recherche en Astrophysique et Planélogie (IRAP - France)
%Copyright          IRAP UPS/CNRS
%Doc.User           http://cassis.irap.omp.eu
%ReleaseNumber      6.3.0.0 - 2022 (Aladin Plugin)
%Plugin             http://cassis.irap.omp.eu/download/CassisPAl-latest.jar
%Aladin.Activated   Yes
%JavaParam          cassis
%Aladin.VOLabel     CASSIS spectrum analyser [IRAP/OVGSO]
%Aladin.Profile     >=12.00

%ActionName         CASSIS-6.2
%Description        CASSIS interactive spectrum analyser (plugin version)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1665996628  2022/10/17 10:50:28
%VerboseDescr       The CASSIS (Centre d'Analyse Scientifique de Spectres Instrumentaux et Synthéques) software has been developed by CESR/IRAP since 2005. CASSIS uses the SSAP (Single Spectral Access Protocol) and EPN-TAP (EuroPlaNet Table Access Protocol) protocols to access the IVOA services in order to retrieve any spectra (Hubble, Corot, Splatalogue, ISO, etc; the complete list dans be found at http://registry.euro-vo.org webpage) via our SSAP or EPN-TAP module. You can also process to line identification using the VAMDC (Virtual And Molecular Database Center) or SLAP (Simple Line Access Protocol) protocols. Of course, CASSIS uses the SAMP messaging protocol (Simple Application Messaging Protocol) that enables astronomy software tools to interoperate and communicate.
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%VersionNumber      1576074585  2019/12/11 16:29:45
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%Param.Value        $7=ARC
%Param.Value        $7=AIT
%Param.Value        $7=ZEA
%Param.Value        $7=CAR
%Param.Value        $7=ZPN
%Param.Value        $7=MOL
%Param.Value        $7=FIE
%Param.Value        $7=GLS
%Param.Value        $8=0.0
%Param.Value        $9=ALL
%Param.Value        $9=ASTRON/P/apertif_dr1
%Param.Value        $9=CDS/P/2MASS
%Param.Value        $9=CDS/P/2MASS6X
%Param.Value        $9=CDS/P/AKARI
%Param.Value        $9=CDS/P/ATLASGAL
%Param.Value        $9=CDS/P/CFHTLS
%Param.Value        $9=CDS/P/CO
%Param.Value        $9=CDS/P/COHRS
%Param.Value        $9=CDS/P/DECaLS
%Param.Value        $9=CDS/P/DECaPS
%Param.Value        $9=CDS/P/DES-DR1
%Param.Value        $9=CDS/P/DM
%Param.Value        $9=CDS/P/DSS2
%Param.Value        $9=CDS/P/EGRET
%Param.Value        $9=CDS/P/Fermi
%Param.Value        $9=CDS/P/Finkbeiner
%Param.Value        $9=CDS/P/GALEXGR6
%Param.Value        $9=CDS/P/GalaxyCounts
%Param.Value        $9=CDS/P/HI
%Param.Value        $9=CDS/P/HI4PI
%Param.Value        $9=CDS/P/HLA
%Param.Value        $9=CDS/P/HSC
%Param.Value        $9=CDS/P/HST
%Param.Value        $9=CDS/P/Haslam408
%Param.Value        $9=CDS/P/INTGAL
%Param.Value        $9=CDS/P/IPHAS
%Param.Value        $9=CDS/P/ISOPHOT
%Param.Value        $9=CDS/P/JPSPR1
%Param.Value        $9=CDS/P/MAMA
%Param.Value        $9=CDS/P/MSX
%Param.Value        $9=CDS/P/Mars
%Param.Value        $9=CDS/P/NEOWISER
%Param.Value        $9=CDS/P/NVSS
%Param.Value        $9=CDS/P/PLANCK
%Param.Value        $9=CDS/P/PanSTARRS
%Param.Value        $9=CDS/P/RASS
%Param.Value        $9=CDS/P/ROSATWFC
%Param.Value        $9=CDS/P/SCUBA
%Param.Value        $9=CDS/P/SCUBA2
%Param.Value        $9=CDS/P/SDSS9
%Param.Value        $9=CDS/P/SHASSA
%Param.Value        $9=CDS/P/SHS
%Param.Value        $9=CDS/P/SPITZER
%Param.Value        $9=CDS/P/SUMSS
%Param.Value        $9=CDS/P/TESS
%Param.Value        $9=CDS/P/THOR
%Param.Value        $9=CDS/P/ULTRAVISTA
%Param.Value        $9=CDS/P/VISTA
%Param.Value        $9=CDS/P/VLSSr
%Param.Value        $9=CDS/P/VTSS
%Param.Value        $9=CDS/P/Venus
%Param.Value        $9=CDS/P/WENSS
%Param.Value        $9=CDS/P/WISE
%Param.Value        $9=CDS/P/WMAP
%Param.Value        $9=CDS/P/allWISE
%Param.Value        $9=CDS/P/skymapper-G
%Param.Value        $9=CDS/P/skymapper-I
%Param.Value        $9=CDS/P/skymapper-R
%Param.Value        $9=CDS/P/skymapper-U
%Param.Value        $9=CDS/P/skymapper-V
%Param.Value        $9=CDS/P/skymapper-Z
%Param.Value        $9=CDS/P/unWISE
%Param.Value        $9=China-VO/P/Change2
%Param.Value        $9=ESAVO/P/AKARI
%Param.Value        $9=ESAVO/P/EXOSAT
%Param.Value        $9=ESAVO/P/HERSCHEL
%Param.Value        $9=ESAVO/P/Haslam408
%Param.Value        $9=ESAVO/P/Haslam_2014
%Param.Value        $9=ESAVO/P/INTEGRAL
%Param.Value        $9=ESAVO/P/ISO
%Param.Value        $9=ESAVO/P/PLANCK
%Param.Value        $9=ESAVO/P/Planck-2015-Pol-Dust
%Param.Value        $9=ESAVO/P/Planck-2015-Pol-Synchrotron
%Param.Value        $9=JAXA/P/bice
%Param.Value        $9=Leiden/P/TGSSADR
%Param.Value        $9=hips.astron.nl/P/tgssadr
%Param.Value        $9=idoc/P/omega
%Param.Value        $9=jvo/P/spcam
%Param.Value        $9=nasa.heasarc/P/Swift
%Param.Value        $9=ov-gso/P/AKARI
%Param.Value        $9=ov-gso/P/AMIGPS
%Param.Value        $9=ov-gso/P/Abell1763
%Param.Value        $9=ov-gso/P/BAT
%Param.Value        $9=ov-gso/P/BLAST
%Param.Value        $9=ov-gso/P/BOLOCAM
%Param.Value        $9=ov-gso/P/C2D
%Param.Value        $9=ov-gso/P/CC
%Param.Value        $9=ov-gso/P/CGPS
%Param.Value        $9=ov-gso/P/CHIPASS
%Param.Value        $9=ov-gso/P/CLASH
%Param.Value        $9=ov-gso/P/COMPTEL
%Param.Value        $9=ov-gso/P/Cygnus
%Param.Value        $9=ov-gso/P/DEBRIS
%Param.Value        $9=ov-gso/P/DIRBE
%Param.Value        $9=ov-gso/P/DRAO-VillaElisa
%Param.Value        $9=ov-gso/P/DRAO
%Param.Value        $9=ov-gso/P/DUSTiNGS
%Param.Value        $9=ov-gso/P/DWINGELOO
%Param.Value        $9=ov-gso/P/Dunes
%Param.Value        $9=ov-gso/P/EBHIS
%Param.Value        $9=ov-gso/P/EFFELSBERG+EMLS
%Param.Value        $9=ov-gso/P/EFFELSBERG
%Param.Value        $9=ov-gso/P/ELFLock
%Param.Value        $9=ov-gso/P/EPoS
%Param.Value        $9=ov-gso/P/FIDEL
%Param.Value        $9=ov-gso/P/FLS
%Param.Value        $9=ov-gso/P/Fermi
%Param.Value        $9=ov-gso/P/Frontier
%Param.Value        $9=ov-gso/P/GASS
%Param.Value        $9=ov-gso/P/GAURIBIDANUR
%Param.Value        $9=ov-gso/P/GLEAM
%Param.Value        $9=ov-gso/P/GLIMPSE
%Param.Value        $9=ov-gso/P/GOALS
%Param.Value        $9=ov-gso/P/GOODS
%Param.Value        $9=ov-gso/P/Gould
%Param.Value        $9=ov-gso/P/HI4PI
%Param.Value        $9=ov-gso/P/HIPASS-ZOA
%Param.Value        $9=ov-gso/P/HLS
%Param.Value        $9=ov-gso/P/HRS
%Param.Value        $9=ov-gso/P/Hatlas
%Param.Value        $9=ov-gso/P/HeViCS
%Param.Value        $9=ov-gso/P/Helga
%Param.Value        $9=ov-gso/P/HerM33es
%Param.Value        $9=ov-gso/P/Heritage
%Param.Value        $9=ov-gso/P/Hermes
%Param.Value        $9=ov-gso/P/Higal
%Param.Value        $9=ov-gso/P/Hobys
%Param.Value        $9=ov-gso/P/ID1600773792
%Param.Value        $9=ov-gso/P/INTEGRAL
%Param.Value        $9=ov-gso/P/IRIS
%Param.Value        $9=ov-gso/P/IRTS
%Param.Value        $9=ov-gso/P/Kingfish
%Param.Value        $9=ov-gso/P/LAB
%Param.Value        $9=ov-gso/P/LG
%Param.Value        $9=ov-gso/P/LVL
%Param.Value        $9=ov-gso/P/M31
%Param.Value        $9=ov-gso/P/MAIPU-MU
%Param.Value        $9=ov-gso/P/MIPSGAL
%Param.Value        $9=ov-gso/P/MITEoR
%Param.Value        $9=ov-gso/P/Madden
%Param.Value        $9=ov-gso/P/Meisenheimer
%Param.Value        $9=ov-gso/P/Nobeyama
%Param.Value        $9=ov-gso/P/PARKES
%Param.Value        $9=ov-gso/P/PILOT
%Param.Value        $9=ov-gso/P/RASS
%Param.Value        $9=ov-gso/P/S4G
%Param.Value        $9=ov-gso/P/SAG4
%Param.Value        $9=ov-gso/P/SAGE
%Param.Value        $9=ov-gso/P/SAGE_irac2
%Param.Value        $9=ov-gso/P/SCANDELS
%Param.Value        $9=ov-gso/P/SCOSMOS
%Param.Value        $9=ov-gso/P/SDWFS
%Param.Value        $9=ov-gso/P/SEP
%Param.Value        $9=ov-gso/P/SERVS
%Param.Value        $9=ov-gso/P/SGPS
%Param.Value        $9=ov-gso/P/SHASSA
%Param.Value        $9=ov-gso/P/SINGS
%Param.Value        $9=ov-gso/P/SMOG
%Param.Value        $9=ov-gso/P/SMUVS
%Param.Value        $9=ov-gso/P/SRELICS
%Param.Value        $9=ov-gso/P/STOCKERT+VILLAELISA
%Param.Value        $9=ov-gso/P/STOCKERT
%Param.Value        $9=ov-gso/P/SUMSS
%Param.Value        $9=ov-gso/P/SWIRE
%Param.Value        $9=ov-gso/P/SpIES
%Param.Value        $9=ov-gso/P/SpUDS
%Param.Value        $9=ov-gso/P/Taurus
%Param.Value        $9=ov-gso/P/URUMQI
%Param.Value        $9=ov-gso/P/VELACAR
%Param.Value        $9=ov-gso/P/VELACAR_irac1
%Param.Value        $9=ov-gso/P/VGPS
%Param.Value        $9=ov-gso/P/VLSSr
%Param.Value        $9=ov-gso/P/VNGS
%Param.Value        $9=ov-gso/P/VTSS
%Param.Value        $9=ov-gso/P/WHAM
%Param.Value        $9=wfau.roe.ac.uk/P/UHSDR1
%Param.Value        $9=wfau.roe.ac.uk/P/UKIDSS
%Param.Value        $9=xcatdb/P/XMM
%Param.Value        $10=ALL
%Param.Value        $10=apertif_dr1
%Param.Value        $10=2MASS
%Param.Value        $10=2MASS6X
%Param.Value        $10=AKARI
%Param.Value        $10=ATLASGAL
%Param.Value        $10=CFHTLS
%Param.Value        $10=CO
%Param.Value        $10=COHRS
%Param.Value        $10=DECaLS
%Param.Value        $10=DECaPS
%Param.Value        $10=DES-DR1
%Param.Value        $10=DM
%Param.Value        $10=DSS2
%Param.Value        $10=EGRET
%Param.Value        $10=Fermi
%Param.Value        $10=Finkbeiner
%Param.Value        $10=GALEXGR6
%Param.Value        $10=GalaxyCounts
%Param.Value        $10=HI
%Param.Value        $10=HI4PI
%Param.Value        $10=HLA
%Param.Value        $10=HSC
%Param.Value        $10=HST
%Param.Value        $10=Haslam408
%Param.Value        $10=INTGAL
%Param.Value        $10=IPHAS
%Param.Value        $10=ISOPHOT
%Param.Value        $10=JPSPR1
%Param.Value        $10=MAMA
%Param.Value        $10=MSX
%Param.Value        $10=Mars
%Param.Value        $10=NEOWISER
%Param.Value        $10=NVSS
%Param.Value        $10=PLANCK
%Param.Value        $10=PanSTARRS
%Param.Value        $10=RASS
%Param.Value        $10=ROSATWFC
%Param.Value        $10=SCUBA
%Param.Value        $10=SCUBA2
%Param.Value        $10=SDSS9
%Param.Value        $10=SHASSA
%Param.Value        $10=SHS
%Param.Value        $10=SPITZER
%Param.Value        $10=SUMSS
%Param.Value        $10=TESS
%Param.Value        $10=THOR
%Param.Value        $10=ULTRAVISTA
%Param.Value        $10=VISTA
%Param.Value        $10=VLSSr
%Param.Value        $10=VTSS
%Param.Value        $10=Venus
%Param.Value        $10=WENSS
%Param.Value        $10=WISE
%Param.Value        $10=WMAP
%Param.Value        $10=allWISE
%Param.Value        $10=skymapper-G
%Param.Value        $10=skymapper-I
%Param.Value        $10=skymapper-R
%Param.Value        $10=skymapper-U
%Param.Value        $10=skymapper-V
%Param.Value        $10=skymapper-Z
%Param.Value        $10=unWISE
%Param.Value        $10=Change2
%Param.Value        $10=AKARI
%Param.Value        $10=EXOSAT
%Param.Value        $10=HERSCHEL
%Param.Value        $10=Haslam408
%Param.Value        $10=Haslam_2014
%Param.Value        $10=INTEGRAL
%Param.Value        $10=ISO
%Param.Value        $10=PLANCK
%Param.Value        $10=Planck-2015-Pol-Dust
%Param.Value        $10=Planck-2015-Pol-Synchrotron
%Param.Value        $10=bice
%Param.Value        $10=TGSSADR
%Param.Value        $10=tgssadr
%Param.Value        $10=omega
%Param.Value        $10=spcam
%Param.Value        $10=Swift
%Param.Value        $10=AKARI
%Param.Value        $10=AMIGPS
%Param.Value        $10=Abell1763
%Param.Value        $10=BAT
%Param.Value        $10=BLAST
%Param.Value        $10=BOLOCAM
%Param.Value        $10=C2D
%Param.Value        $10=CC
%Param.Value        $10=CGPS
%Param.Value        $10=CHIPASS
%Param.Value        $10=CLASH
%Param.Value        $10=COMPTEL
%Param.Value        $10=Cygnus
%Param.Value        $10=DEBRIS
%Param.Value        $10=DIRBE
%Param.Value        $10=DRAO-VillaElisa
%Param.Value        $10=DRAO
%Param.Value        $10=DUSTiNGS
%Param.Value        $10=DWINGELOO
%Param.Value        $10=Dunes
%Param.Value        $10=EBHIS
%Param.Value        $10=EFFELSBERG+EMLS
%Param.Value        $10=EFFELSBERG
%Param.Value        $10=ELFLock
%Param.Value        $10=EPoS
%Param.Value        $10=FIDEL
%Param.Value        $10=FLS
%Param.Value        $10=Fermi
%Param.Value        $10=Frontier
%Param.Value        $10=GASS
%Param.Value        $10=GAURIBIDANUR
%Param.Value        $10=GLEAM
%Param.Value        $10=GLIMPSE
%Param.Value        $10=GOALS
%Param.Value        $10=GOODS
%Param.Value        $10=Gould
%Param.Value        $10=HI4PI
%Param.Value        $10=HIPASS-ZOA
%Param.Value        $10=HLS
%Param.Value        $10=HRS
%Param.Value        $10=Hatlas
%Param.Value        $10=HeViCS
%Param.Value        $10=Helga
%Param.Value        $10=HerM33es
%Param.Value        $10=Heritage
%Param.Value        $10=Hermes
%Param.Value        $10=Higal
%Param.Value        $10=Hobys
%Param.Value        $10=ID1600773792
%Param.Value        $10=INTEGRAL
%Param.Value        $10=IRIS
%Param.Value        $10=IRTS
%Param.Value        $10=Kingfish
%Param.Value        $10=LAB
%Param.Value        $10=LG
%Param.Value        $10=LVL
%Param.Value        $10=M31
%Param.Value        $10=MAIPU-MU
%Param.Value        $10=MIPSGAL
%Param.Value        $10=MITEoR
%Param.Value        $10=Madden
%Param.Value        $10=Meisenheimer
%Param.Value        $10=Nobeyama
%Param.Value        $10=PARKES
%Param.Value        $10=PILOT
%Param.Value        $10=RASS
%Param.Value        $10=S4G
%Param.Value        $10=SAG4
%Param.Value        $10=SAGE
%Param.Value        $10=SAGE_irac2
%Param.Value        $10=SCANDELS
%Param.Value        $10=SCOSMOS
%Param.Value        $10=SDWFS
%Param.Value        $10=SEP
%Param.Value        $10=SERVS
%Param.Value        $10=SGPS
%Param.Value        $10=SHASSA
%Param.Value        $10=SINGS
%Param.Value        $10=SMOG
%Param.Value        $10=SMUVS
%Param.Value        $10=SRELICS
%Param.Value        $10=STOCKERT+VILLAELISA
%Param.Value        $10=STOCKERT
%Param.Value        $10=SUMSS
%Param.Value        $10=SWIRE
%Param.Value        $10=SpIES
%Param.Value        $10=SpUDS
%Param.Value        $10=Taurus
%Param.Value        $10=URUMQI
%Param.Value        $10=VELACAR
%Param.Value        $10=VELACAR_irac1
%Param.Value        $10=VGPS
%Param.Value        $10=VLSSr
%Param.Value        $10=VNGS
%Param.Value        $10=VTSS
%Param.Value        $10=WHAM
%Param.Value        $10=UHSDR1
%Param.Value        $10=UKIDSS
%Param.Value        $10=XMM
%Param.Value        $11=application/fits
%Param.Value        $11=image/jpeg
%Param.Value        $11=image/png
%ResultDataType        Mime(image/xml)
%VerboseDesc        Aladin SIAv2 service (based on Hips2Fits cutout service)..
%Aladin.Profile     >11.036 beta
%Aladin.Logo        AladinSIAv2.png
%Aladin.XLabel      HiPSi2Fits\nSIAv2
%Aladin.LabelPlane  HiPS-CDS SIAv2 $1 $2

%ActionName         Hips2Fits
%Description        Aladin HiPS to Fits cutout service  form
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                <&Hips2FitsU>?ra=$1&dec=$2&fov=$3&hips=$4&width=$5&height=$5&coordsys=$6&projection=$7&rotation_angle=0&format=$8
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=FoV (deg)
%Param.Description  $4=Survey (ID or keyword)
%Param.Description  $5=Size (pix)
%Param.Description  $6=Coord.sys
%Param.Description  $7=Projection
%Param.Description  $8=Format
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.Value        $4=CDS/P/2MASS/J
%Param.Value        $5=1024
%Param.Value        $6=icrs
%Param.Value        $6=galactic
%Param.Value        $7=SIN - orthographic
%Param.Value        $7=TAN - tangential
%Param.Value        $7=MOL - Mollweide
%Param.Value        $7=AIT - Hammer-Aitoff
%Param.Value        $7=STG - stereographic
%Param.Value        $7=ARC - zenithal/azimuthal equidistant
%Param.Value        $7=ZEA - zenithal/azimuthal equal area
%Param.Value        $7=AZP - zenithal/azimuthal perspective
%Param.Value        $7=SZP - slant zenithal perspective
%Param.Value        $7=AIR - Airy's projection
%Param.Value        $7=CYP - cylindrical perspective
%Param.Value        $7=CEA - cylindrical equal area
%Param.Value        $7=CAR - plate carr&eacute;e
%Param.Value        $7=MER - Mercator
%Param.Value        $7=SFL - Sanson-Flamsteed
%Param.Value        $7=PAR - parabolic
%Param.Value        $7=TSC - tangential spherical cube
%Param.Value        $7=CSC - COBE spherical cube
%Param.Value        $7=QSC - quadrilateralized spherical cube
%Param.Value        $7=HPX - HEALPix
%Param.Value        $7=XPH - HEALPix polar, "butterfly"
%Param.Value        $8=fits - Full dynamic
%Param.Value        $8=jpg - JPEG ompressed, 8 bits
%Param.Value        $8=png - Compressed, 8 bits
%ResultDataType     Mime(image)
%Doc.User            http://alaskybis.cds.unistra.fr/hips-image-services/hips2fits
%Aladin.Profile     >10.140
%Aladin.Label       Aladin
%Aladin.Logo        AladinHips2fits.png
%Aladin.LabelPlane  Hips2fits $4
%Aladin.MenuNumber  I2

%ActionName         Hips2FitsU
%Description        Aladin HiPS cutout service URL  prefix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1746890968  2025/05/10 17:29:28
%SeeAction          Hips2FitsU.alaskybis
%SeeAction          Hips2FitsU.alasky

%ActionName         Http
%Description        Usage of GLU to query remotely an other httpd
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1396271783  2014/03/31 15:16:23
%Url                $1

%ActionName         HttpGluGateway
%Description        HTTP GLU gateways. Glu sites "queryable" via HTTP (for applications such as Aladin)
%Owner              CDS'glu
%DistribDomain      CDS
%VersionNumber      2  2003/05/20 15:55:33
%SeeAction          HttpGluGateway.ch availability=14
%SeeAction          HttpGluGateway.ru availability=9999
%SeeAction          HttpGluGateway.iucaa availability=9999
%SeeAction          HttpGluGateway.adac availability=12
%SeeAction          HttpGluGateway.cadc availability=9999
%SeeAction          HttpGluGateway.uk availability=10
%SeeAction          HttpGluGateway.cfa availability=17
%SeeAction          HttpGluGateway.cds availability=0

%ActionName         HttpGluGateway.hw
%Description        Hawaii HTTP GLU gateway (for applications such as Aladin).
%Owner              CDS'glu
%DistribDomain      CDS
%VersionNumber      2  2003/05/20 18:02:55
%Url                http://www.ukirt.jach.hawaii.edu/viz-bin/nph-glu.pl?$1
%Param.Description  $1=Glu tag or Glu ID

%ActionName         I-259-tyc2.hpx
%Description        Tycho2 progressive catalog
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/cats/Tycho2
%Id                 I/259/tyc2
%Aladin.Profile     >6.1 <8.159
%Aladin.XLabel      Tycho2
%Aladin.Tree        Progressive catalog
%Aladin.HpxParam    6 cat
%VerboseDesc        Tycho2 hierarchical access

%ActionName         I-312.hpx
%Description        PPMX progressive catalog
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/cats/PPMX
%Id                 I/312
%Aladin.Profile     >=6.1 <8.159
%Aladin.HpxParam    9 cat
%Aladin.XLabel      PPMX
%Aladin.Tree        Progressive catalog
%VerboseDesc        PPMX hierarchical access

%ActionName         I/324.hpx
%Description        IGLS3 progressive catalog (I/324)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/HipsCatService/IGLS3/
%Copyright          beta acces only
%Id                 I/324
%Aladin.Profile     >6.1 <8.159 beta
%Aladin.XLabel      IGSL3
%Aladin.Tree        Progressive catalog
%Aladin.HpxParam    11 cat equatorial
%VerboseDesc        IGLS3 hierarchical access

%ActionName         IAU-Directory
%Description        International Astronomical Union: Addresses of members
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      0  1998/02/16 18:24:43
%Url                http://www.astro.ku.dk/cgi-bin/iau_mem.cgi?name=$1&Action=Search
%Param.Description  $1=Last name of Astronomy person
%Param.DataType     $1=CDS'misc'query/name
%ResultDataType     Mime(text/html)
%Doc.User           http://www.intastun.org/

%ActionName         IBVS.fullpaper
%Description        Information Bulletin on Variable Stars
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1316448247  2011/09/19 18:04:07
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%ActionName         II-294.hpx
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%Url                http://alasky.cds.unistra.fr/cats/AKARI_FIS
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%ActionName         IMCCE
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%ActionName         IMCCE.aster
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%Url                http://vo.imcce.fr/webservices/miriade/ephemcc_query.php?-from=VizieR&-tscale=UTC&-mime=html&-tcoor=1&-step=1d&-nbd=1&-ep=now&-observer=500&-name=a:$1
%Param.Description  $1=Asteroid Name
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%ActionName         IMCCE.comet
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%Param.Description  $1=Asteroid Name
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%ActionName         IMCCE.planet
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%Url                http://www.imcce.fr/cgi-bin/select_ephepos.cgi/calcul?planete=$1&numaster=&nomaster=&nomcomet=&an=$2&mois=$3&jour=$4&heure=12&minutes=00&secondes=00&nbdates=15&pas=1.0&codepas=1&keph=5&centre=2&site=3&pr=1&tc=1&te=1
%Param.Description  $1=Planet Name
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%ActionName         INASAN.home
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%VersionNumber      1340094952  2012/06/19 10:35:52
%Url                http://www.inasan.ru/
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%ActionName         INES.home
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%Url                http://ines.laeff.esa.es/ines/
%DefaultAnchorText  INES (IUE Newly Extracted Spectra)
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%ActionName         INES.sp
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%ActionName         INES.sp.fr
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%ActionName         INSU.home
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%Url                http://www.insu.cnrs.fr/
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%ActionName         IRIS100.hpx.outreach
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%Url                http://alasky.cds.unistra.fr/IRIS_4
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%ActionName         IRISColor.hpx.outreach
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%ActionName         IRODS-test
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%ActionName         ISO.jsp
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%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://ida.esac.esa.int:8080/aio/jsp/createPostcards.jsp?obsno=$1
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%ActionName         IUCAA.home
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%ActionName         IUEQuery
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%ActionName         IVOA.home
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%ActionName         Image.GOODS
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%Url                http://aladin.u-strasbg.fr/cgi-bin/nph-HTTP1.cgi?out=IMAGE&mode=VIEW&position=$1&survey=$2&color=$3&field=$4&comp=NONE

%ActionName         Interop.menu
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%ActionName         Java.home
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%ActionName         JavaInfo
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%Url                http://aladin.cds.unistra.fr/java/JavaInfo.htx
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%ActionName         Jodrell.home
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%Url                http://www.jb.man.ac.uk/
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%ActionName         JournalList
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%ActionName         LAM.home
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%ActionName         LEDA
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%Url                http://leda.univ-lyon1.fr/leda-aladin.cgi?type=astrores&ra=$1&de=$2&width=$3&height=$4&constraint=$5
%Param.Description  $1=Right Ascension
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%ActionName         LSIIT.home
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%VersionNumber      1  2001/12/31 15:08:19
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%ActionName         MACHO.data
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%Url                http://store.anu.edu.au:3001/cgi-bin/clclite?star=$1.$2.$3&sodset=PhotSS/F_$1/sodset_$1.$2&List=Extract
%Param.Description  $1=field
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%ActionName         MACHO.home
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%Owner              CDS'VizieR
%DistribDomain      CDS
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%Url                http://wwwmacho.mcmaster.ca/Data/MachoData.html
%ResultDataType     Mime(text/html)

%ActionName         MACHO.plot
%Description        Get light variation of stars in MACHO
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://store.anu.edu.au:3001/cgi-bin/clclite?star=$1.$2.$3&sodset=PhotSS/F_$1/sodset_$1.$2&Action=Submit
%Param.Description  $1=field
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%Param.Value        $1=1
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%ActionName         MAST
%Description        Multimission Archive at STScI (MAST)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576257920  2019/12/13 19:25:20
%Url                http://archive.stsci.edu/siap/search.php?FORMAT=image/fits&POS=$1,$2&SIZE=$3,$4&ID=$5
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Width (deg)
%Param.Description  $4=Height (deg)
%Param.Description  $5=mission/instrument
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
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%Param.DataType     $4=Field(DEd)
%Param.Value        $3=0.17
%Param.Value        $4=0.17
%Param.Value        $5=ALL - Search all missions
%Param.Value        $5=   GALEX - Galaxy Evolution Explorer
%Param.Value        $5=   HST - All Hubble Space Telescope Previews
%Param.Value        $5=      STIS - Space Telescope Imaging Spectrograph Previews
%Param.Value        $5=      ACS - Advanced Camera for Survey Previews
%Param.Value        $5=      NICMOS - Near IR Camera & Multi Object Spectrometer Previews
%Param.Value        $5=      WFPC - Wide Field Planetary Camera Previews
%Param.Value        $5=      WFPC2 - Wide Field Planetary Camera 2 Previews
%Param.Value        $5=      FOC - Faint Object Camera Previews
%Param.Value        $5=   UIT - Ultraviolet Imaging Telescope
%Param.Value        $5=   VLA-FIRST - VLA Faint Radio Images at 21 cm
%Param.Value        $5=   XMM-OM - XMM Optical Monitor Images
%Param.Value        $5=   HLSP - All High Level Science Products
%Param.Value        $5=      GOODS - Great Observatories Origins Deep Survey
%Param.Value        $5=      TNO - Trans-Neptunian Objects Search Field
%Param.Value        $5=      UDF - Hubble Ultra Deep Field
%Param.Value        $5=      UDF05 - Hubble Ultra Deep Field Follow-Up
%Param.Value        $5=      HDF - Hubble Deep Field
%Param.Value        $5=      HDF_SOUTH - Hubble Deep Field South
%Param.Value        $5=      MAOZ_ATLAS - HST UV Images of Nearby Galaxies
%Param.Value        $5=      HELIX - HST images of the Helix Nebula
%Param.Value        $5=      APPP - WFPC2 Pure Parallel Program
%Param.Value        $5=      GEMS - Galaxy Evolution from Morphology and SEDs
%Param.Value        $5=      M51 - Multi-color ACS mosaic of the M51 Galaxy
%Param.Value        $5=      SGAL - WFPC2 Spiral Galaxies
%Param.Value        $5=      COSMOS - HST Cosmic Evolution Survey
%Param.Value        $5=      GALEX_ATLAS - GALEX Atlas of Nearby Galaxies
%ResultDataType     Mime(sia/xml)
%VerboseDescr       Allows access (via SIAP) to HST preview images (including STIS, WFPC, WFPC2, NICMOS, ACS and FOC), GALEX, UIT, VLA-FIRST, XMM-OM and various High Level Science Products (HLSPs)
%Institute          Multimission Archive at Space Telescope Science Institute
%Doc.User           http://archive.stsci.edu/siap/help/search_help.html
%Aladin.Menu        Archives...
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%Aladin.Logo        MASTLogo.gif
%Aladin.LabelPlane  MAST $4

%ActionName         MNRAS.fullpaper
%Description        Astronomical Journal article
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%VersionNumber      1242041213  2009/05/11 13:26:53
%Url                http://cds.u-strasbg.fr/cgi-bin/nph-doi?$1
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%ActionName         MNRAS.logo
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%Url                https://ned.ipac.caltech.edu/tap/sync?REQUEST=doQuery&LANG=ADQL&MAXREC=1000000&QUERY=SELECT+TOP+999999+*+FROM+NEDTAP.objdir+WHERE+CONTAINS%28POINT%28%27ICRS%27%2C+ra%2C+dec%29%2C+CIRCLE%28%27ICRS%27%2C+$1%2C+$2%2C+$3%29%29+%3D+1
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%VerboseDescr       The NASA/IPAC Extragalactic Database (NED) is built around a master list of extragalactic objects for which cross-identifications of names have been established, accurate positions and redshifts entered to the extent possible, and some basic data collected.  Bibliographic references relevant to individual objects have been compiled, and abstracts of extragalactic interest are kept on line
%Doc.User           http://nedwww.ipac.caltech.edu/help/intro.html
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%Aladin.XLabel      NASA/IPAC Extragalactic Database (Caltech/Pasadena)
%Aladin.Profile     >10.05
%Aladin.Filter      #All objects\nfilter All { ${pretype}="G" { draw oval }\n${pretype}="RadioS" || ${pretype}="Maser" { draw triangle }\n${pretype}="IRS" || ${pretype}="IrS" {draw rhomb}\n${pretype}="\\*" {draw circle(3)}\n${pretype}="Vis*" ||${pretype}="SNR" || ${pretype}="Neb" || ${pretype}="HI*" {draw square}\n${pretype}="UV*" {draw cross;draw plus}\n${pretype}="X*" {draw cross}\n{ draw ${pretype} }  }
%Aladin.Filter      #Star\nfilter Star { ${pretype}="\\*" {draw circle(3)} }
%Aladin.Filter      #Galaxy\nfilter Galaxy { ${pretype}="G" { draw oval } }
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%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/2MASS/H
%VerboseDescr       2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF
%Copyright          University of Massachusetts & IPAC/Caltech
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%Id                 P/2MASS/H
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%SkyFraction        1
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%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/2MASS/J
%VerboseDescr       2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS/J
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/
%SkyFraction        1
%Aladin.XLabel      The Two Micron All Sky Survey - J band (2MASS J)
%Aladin.Tree        Image/Infrared/2MASS
%Aladin.MenuNumber  04-001-02
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2016-04-22T14:03Z

%ActionName         P-2MASS-K.hpx
%Description        2MASS K (2.16um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/2MASS/K
%VerboseDescr       2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS/K
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/
%SkyFraction        1
%Aladin.XLabel      The Two Micron All Sky Survey - K band (2MASS K)
%Aladin.Tree        Image/Infrared/2MASS
%Aladin.MenuNumber  04-001-04
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2016-04-22T14:23Z

%ActionName         P-2MASS-color.hpx
%Description        2MASS color J (1.23um), H (1.66um), K (2.16um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-2MASS-color_0.hpx availability=0
%SeeAction          P-2MASS-color_1.hpx availability=11
%SeeAction          P-2MASS-color_2.hpx availability=0
%SeeAction          P-2MASS-color_3.hpx availability=0
%SeeAction          P-2MASS-color_4.hpx availability=9999
%SeeAction          P-2MASS-color_5.hpx availability=19
%VerboseDescr       2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/
%SkyFraction        1
%Aladin.XLabel      The Two Micron All Sky Survey - J-H-K bands (2MASS color)
%Aladin.Tree        Image/Infrared/2MASS
%Aladin.MenuNumber  04-001-00 lite
%Aladin.HpxParam    9 image color equatorial jpeg
%Aladin.Date        2016-04-22T14:40Z

%ActionName         P-2MASS6X-H.hpx
%Description        2MASS6X H (1.66um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/2MASS6X/2MASS6X_H
%VerboseDescr       During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS6X/H
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html
%SkyFraction        0.01316
%Aladin.XLabel      2MASS6X H
%Aladin.Tree        Image/Infrared/2MASS/2MASS6X
%Aladin.MenuNumber  04-001-99-02
%Aladin.HpxParam    9 image equatorial png jpeg fits
%Aladin.Date        2017-03-28T09:34Z

%ActionName         P-2MASS6X-J.hpx
%Description        2MASS6X J (1.23um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/2MASS6X/2MASS6X_J
%VerboseDescr       During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS6X/J
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html
%SkyFraction        0.01316
%Aladin.XLabel      2MASS6X J
%Aladin.Tree        Image/Infrared/2MASS/2MASS6X
%Aladin.MenuNumber  04-001-99-01
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:41Z

%ActionName         P-2MASS6X-K.hpx
%Description        2MASS6X K (2.16um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/2MASS6X/2MASS6X_K
%VerboseDescr       During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS6X/K
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html
%SkyFraction        0.01316
%Aladin.XLabel      2MASS6X K
%Aladin.Tree        Image/Infrared/2MASS/2MASS6X
%Aladin.MenuNumber  04-001-99-03
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:43Z

%ActionName         P-2MASS6X-color.hpx
%Description        2MASS6X color J (1.23um) & K (2.16um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/2MASS6X/2MASS6X_color
%VerboseDescr       During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/2MASS6X/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html
%SkyFraction        0.01316
%Aladin.XLabel      2MASS6X color
%Aladin.Tree        Image/Infrared/2MASS/2MASS6X
%Aladin.MenuNumber  04-001-99-00
%Aladin.HpxParam    9 image color equatorial png
%Aladin.Date        2017-03-28T12:31Z

%ActionName         P-AKARI-FIS-Color.hpx
%Description        AKARI FIS Color WideL (140um), WideS (90um), N60 (65um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-AKARI-FIS-Color_0.hpx availability=0
%SeeAction          P-AKARI-FIS-Color_1.hpx availability=0
%SeeAction          P-AKARI-FIS-Color_2.hpx availability=0
%SeeAction          P-AKARI-FIS-Color_3.hpx availability=9999
%VerboseDescr       AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See  http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf.
%Copyright          ISAS/JAXA
%Origin             CDS
%Id                 P/AKARI/FIS/Color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/
%SkyFraction        1
%Aladin.XLabel      AKARI FIS Color
%Aladin.Tree        Image/Infrared/AKARI-FIS
%Aladin.MenuNumber  04-05-00 lite
%Aladin.HpxParam    5 image color equatorial png jpeg
%Aladin.Date        2016-05-26T15:16Z

%ActionName         P-AKARI-FIS-N160.hpx
%Description        AKARI FIS N160 (160um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/AKARI-FIS/N160
%VerboseDescr       AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See  http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf.
%Copyright          ISAS/JAXA
%Origin             CDS
%Id                 P/AKARI/FIS/N160
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/
%SkyFraction        0.9988
%Aladin.XLabel      AKARI FIS N160
%Aladin.Tree        Image/Infrared/AKARI-FIS
%Aladin.MenuNumber  04-05-04
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2016-06-03T12:29Z

%ActionName         P-AKARI-FIS-N60.hpx
%Description        AKARI FIS N60 (65um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/AKARI-FIS/N60
%VerboseDescr       AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See  http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf.
%Copyright          ISAS/JAXA
%Origin             CDS
%Id                 P/AKARI/FIS/N60
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/
%SkyFraction        0.9976
%Aladin.XLabel      AKARI FIS N60
%Aladin.Tree        Image/Infrared/AKARI-FIS
%Aladin.MenuNumber  04-05-01
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2016-06-03T12:30Z

%ActionName         P-AKARI-FIS-WideL.hpx
%Description        AKARI FIS WideL (140um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/AKARI-FIS/WideL
%VerboseDescr       AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See  http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf.
%Copyright          ISAS/JAXA
%Origin             CDS
%Id                 P/AKARI/FIS/WideL
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/
%SkyFraction        0.9989
%Aladin.XLabel      AKARI FIS WideL
%Aladin.Tree        Image/Infrared/AKARI-FIS
%Aladin.MenuNumber  04-05-03
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2016-06-03T12:30Z

%ActionName         P-AKARI-FIS-WideS.hpx
%Description        AKARI FIS WideS (90um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/AKARI-FIS/WideS
%VerboseDescr       AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See  http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf.
%Copyright          ISAS/JAXA
%Origin             CDS
%Id                 P/AKARI/FIS/WideS
%Aladin.Profile     >6.1
%Copyright.Url      http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/
%SkyFraction        0.9976
%Aladin.XLabel      AKARI FIS WideS
%Aladin.Tree        Image/Infrared/AKARI-FIS
%Aladin.MenuNumber  04-05-02
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2016-06-03T12:31Z

%ActionName         P-AMIGPS.hpx
%Description        AMIGPS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/AMIGPS
%VerboseDescr       AMI Galactic Plane Survey at 15.7 GHz, carried out using the Arcminute Microkelvin Imager (AMI) Small Array (SA) and operated by the Cavendish Astrophysics Group at Lord?s Bridge, Cambridgeshire. The angular resolution is approximately 3?. Units: Jy/beam.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/AMIGPS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.04482
%Aladin.XLabel      AMIGPS
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-11-23T13:16Z

%ActionName         P-ASCA_GIS.hpx
%Description        ASCA public data image (256x256)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1500624001  2017/07/21 10:00:01
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/ASCA_GIS
%VerboseDescr       Superposition of GIS pseudo-color images (256x256), no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/ASCA_GIS
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/asca
%SkyFraction        1
%Aladin.XLabel      ASCA_GIS
%Aladin.Tree        Image/X/ASCA
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2016-10-25T07:15Z

%ActionName         P-ASCA_SIS.hpx
%Description        ASCA public data image (SIS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/ASCA_SIS
%VerboseDescr       Superposition of SIS pseudo-color images, no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/ASCA_SIS
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/asca
%SkyFraction        1
%Aladin.XLabel      ASCA_SIS
%Aladin.Tree        Image/X/ASCA
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2016-10-25T07:15Z

%ActionName         P-ATLASGAL-APEXPlanck.hpx
%Description        ATLASGAL APEX-Planck 850um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/APEX/ATLASGAL_APEXPlanck
%VerboseDescr       ATLASGAL is the APEX Telescope Large Area Survey of the Galaxy, an observing programme with the LABOCA bolometer array at APEX, located at 5100 m altitude on Chajnantor, Chile. This survey mapped over 400 square degrees at 870 microns in the inner Galaxy, with a uniform sensitivity of a few solar masses at 1 kpc distance. This project is a collaboration between the Max Planck Gesellschaft (MPG: Max Planck Institute fur Radioastronomie, MPIfR Bonn, and Max Planck Institute fur Astronomie, MPIA Heidelberg), the European Southern Observatory (ESO) and the Universidad de Chile. The APEX telescope is ideally located to observe the inner Milky Way. The Large APEX Bolometer Camera (LABOCA) is a 295-element bolometer array observing at 870 um, with a beam size of 19.2 arcsec. Taking advantage of its large field of view (11.4 arcmin) and excellent sensitivity, we started an unbiased survey of the entire Galactic Plane accessible to APEX, with a typical noise level of 50-70 mJy/beam: the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). The LABOCA data have been combined with the results of the Planck satellite. The method used to combine the Planck and ATLASGAL data together is described in Csengeri et al. (2016).
%Copyright          ESO
%Origin             CDS
%Id                 P/ATLASGAL/APEXPlanck
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.eso.org/cms/eso-data-access-policy.html
%SkyFraction        0.007962
%Aladin.XLabel      ATLASGAL
%Aladin.Tree        Image/Infrared/APEX
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2017-02-20T16:04Z

%ActionName         P-ATLASGAL.hpx
%Description        ATLASGAL 850 um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/APEX/ATLASGAL
%VerboseDescr       ATLASGAL is the APEX Telescope Large Area Survey of the Galaxy, an observing programme with the LABOCA bolometer array at APEX, located at 5100 m altitude on Chajnantor, Chile. This survey mapped over 400 square degrees at 870 microns in the inner Galaxy, with a uniform sensitivity of a few solar masses at 1 kpc distance. This project is a collaboration between the Max Planck Gesellschaft (MPG: Max Planck Institute fur Radioastronomie, MPIfR Bonn, and Max Planck Institute fur Astronomie, MPIA Heidelberg), the European Southern Observatory (ESO) and the Universidad de Chile. The APEX telescope is ideally located to observe the inner Milky Way. The Large APEX Bolometer Camera (LABOCA) is a 295-element bolometer array observing at 870 um, with a beam size of 19.2 arcsec. Taking advantage of its large field of view (11.4 arcmin) and excellent sensitivity, we started an unbiased survey of the entire Galactic Plane accessible to APEX, with a typical noise level of 50-70 mJy/beam: the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL).
%Copyright          ESO
%Origin             CDS
%Id                 P/ATLASGAL
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.eso.org/cms/eso-data-access-policy.html
%SkyFraction        0.01097
%Aladin.XLabel      ATLASGAL
%Aladin.Tree        Image/Infrared/APEX
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2017-02-20T14:25Z

%ActionName         P-Ariel-Voyager.hpx
%Description        Ariel Voyager
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Ariel_Voyager
%VerboseDescr       Ariel Uranus satellite map mosaicked with Voyager imagery by USGS
%Copyright          Caltech/JPL/NASA
%Origin             CDS
%Id                 P/Ariel/Voyager
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Ariel/Voyager
%Aladin.Tree        Solar system/Uranus/Ariel
%Aladin.HpxParam    3 image color ariel jpeg
%Aladin.Date        2018-01-31T06:30Z

%ActionName         P-BASS-DR1-image.hpx
%Description        Beijing-Arizona Sky Survey (BASS) DR1 Image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://hips.china-vo.org/bass-dr1-image
%VerboseDescr       The Beijing-Arizona Sky Survey (BASS) is an ambitious wide-field multicolor survey of 5000 deg^2 of the Northern Galactic Cap using the 90prime imager on the 2.3m Bok Telescope at Kitt Peak, as a three to four-year collaboration between the Chinese team led by NAOC and the US team led by Steward Observatory, University of Arizona. The survey will use 240 nights, covering SDSS g and r bands, reaching limiting AB magnitude of 24.0 and 23.6 (5?), respectively.
%Copyright          Beijing-Arizona Sky Survey (BASS) - NAOC, Healpixed by China-VO
%Origin             China-VO
%Id                 P/BASS/DR1/image
%Aladin.Profile     >6.1
%Copyright.Url      http://batc.bao.ac.cn/BASS/doku.php
%SkyFraction        0.1238
%Aladin.XLabel      BASS DR1 Image
%Aladin.HpxParam    10 image color equatorial png
%Aladin.Date        2017-10-25T19:21Z

%ActionName         P-BASS-DR2-image.hpx
%Description        Beijing-Arizona Sky Survey (BASS) DR2 Image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://hips.china-vo.org/bass-dr2-image
%VerboseDescr       The Beijing-Arizona Sky Survey (BASS) is an ambitious wide-field multicolor survey of 5000 deg^2 of the Northern Galactic Cap using the 90prime imager on the 2.3m Bok Telescope at Kitt Peak, as a three to four-year collaboration between the Chinese team led by NAOC and the US team led by Steward Observatory, University of Arizona. The survey will use 240 nights, covering SDSS g and r bands, reaching limiting AB magnitude of 24.0 and 23.6 (5?), respectively.
%Copyright          Beijing-Arizona Sky Survey (BASS) - NAOC, Healpixed by China-VO
%Origin             China-VO
%Id                 P/BASS/DR2/image
%Aladin.Profile     >6.1
%Copyright.Url      http://batc.bao.ac.cn/BASS/doku.php
%SkyFraction        0.1415
%Aladin.XLabel      BASS DR2 Image
%Aladin.Tree        Image/Optical/BASS
%Aladin.HpxParam    10 image color equatorial png
%Aladin.Date        2017-12-07T16:29Z

%ActionName         P-BAT-100-150keV.hpx
%Description        Swift/BAT 100-150keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_100_150
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 100-150 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/100-150keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
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%Aladin.XLabel      Swift/BAT 100-150keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:10Z

%ActionName         P-BAT-14-20keV.hpx
%Description        Swift/BAT 14-20keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_14_20
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 14-20 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/14-20keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 14-20keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T15:25Z

%ActionName         P-BAT-150-195keV.hpx
%Description        Swift/BAT 150-195keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_150_195
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 150-195 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/150-195keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 150-195keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:16Z

%ActionName         P-BAT-20-24keV.hpx
%Description        Swift/BAT 20-24keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_20_24
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 20-24 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/20-24keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 20-24keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:02Z

%ActionName         P-BAT-24-35keV.hpx
%Description        Swift/BAT 24-35keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_24_35
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 24-35 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/24-35keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 24-35keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:04Z

%ActionName         P-BAT-35-50keV.hpx
%Description        Swift/BAT 35-50keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_35_50
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 35-50 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/35-50keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 35-50keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:05Z

%ActionName         P-BAT-50-75keV.hpx
%Description        Swift/BAT 50-75keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_50_75
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 50-75 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/50-75keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 50-75keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:07Z

%ActionName         P-BAT-75-100keV.hpx
%Description        Swift/BAT 75-100keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BAT_75_100
%VerboseDescr       This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. The energy range is 75-100 keV. Units are counts/sec/detector. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7m2. The angular resolution of the survey is 19.5'. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BAT/75-100keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Swift/BAT 75-100keV
%Aladin.Tree        Image/X-ray/Swift
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-02-20T16:09Z

%ActionName         P-BLAST-250.hpx
%Description        BLAST 250um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BLAST_250
%VerboseDescr       Ballon-borne Large-Aperture Submillimeter Telescope (BLAST)- Survey at 250 mic, at a resolution of 30??. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BLAST/250
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.003738
%Aladin.XLabel      BLAST 250um
%Aladin.Tree        Image/Radio/BLAST
%Aladin.MenuNumber  05-xx
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-12-15T17:56Z

%ActionName         P-BLAST-350.hpx
%Description        BLAST 350um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BLAST_350
%VerboseDescr       Ballon-borne Large-Aperture Submillimeter Telescope (BLAST)- Survey at 350 mic, at a resolution of 42??. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BLAST/350
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.003752
%Aladin.XLabel      BLAST 350um
%Aladin.Tree        Image/Radio/BLAST
%Aladin.MenuNumber  05-xx
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-12-15T17:55Z

%ActionName         P-BLAST-500.hpx
%Description        BLAST 500um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BLAST_500
%VerboseDescr       Ballon-borne Large-Aperture Submillimeter Telescope (BLAST)- Survey at 500 mic, at a resolution of 60??. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BLAST/500
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.003756
%Aladin.XLabel      BLAST_500
%Aladin.Tree        Image/Radio/BLAST
%Aladin.MenuNumber  05-xx
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-12-15T17:51Z

%ActionName         P-BOLOCAM.hpx
%Description        Bolocam Galactic Plane Survey (BGPS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/BOLOCAM
%VerboseDescr       Galactic plane (170 deg2) with an effective resolution of 33" at 1.1 mm. Units: Jy/beam - see 2011ApJS..192....4A
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/BOLOCAM
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.01008
%Aladin.XLabel      Bolocam
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-02
%Aladin.HpxParam    5 image galactic jpeg fits
%Aladin.Date        2013-09-04T13:33Z

%ActionName         P-CFHTLS-D-color-ugi.hpx
%Description        CFHTLS-D-color-ugi
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/RGB-UGIm
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very long exposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/color/ugi
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.009E-4
%Aladin.XLabel      CFHTLS D color ugi
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-00
%Aladin.HpxParam    12 image color equatorial jpeg
%Aladin.Date        2017-03-28T09:09Z

%ActionName         P-CFHTLS-D-g.hpx
%Description        CFHTLS-D-g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/GALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/g
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.044E-4
%Aladin.XLabel      CFHTLS D g
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-02
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2017-03-28T08:57Z

%ActionName         P-CFHTLS-D-i.hpx
%Description        CFHTLS-D-i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/IALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/i
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.044E-4
%Aladin.XLabel      CFHTLS D i
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-04
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:02Z

%ActionName         P-CFHTLS-D-r.hpx
%Description        CFHTLS-D-r
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/RALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/r
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.044E-4
%Aladin.XLabel      CFHTLS D r
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-03
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:04Z

%ActionName         P-CFHTLS-D-u.hpx
%Description        CFHTLS-D-u
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/UALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/u
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.044E-4
%Aladin.XLabel      CFHTLS D u
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-01
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:05Z

%ActionName         P-CFHTLS-D-z.hpx
%Description        CFHTLS-D-z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/ZALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/D/z
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        1.044E-4
%Aladin.XLabel      CFHTLS D z
%Aladin.Tree        Image/Optical/CFHTLS/DEEP
%Aladin.MenuNumber  03-04-02-05
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2017-03-28T09:08Z

%ActionName         P-CFHTLS-W-Color-ugi.hpx
%Description        CFHTLS-W-colored-ugi
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/RGB-UGIm
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/Color/ugi
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W Color ugi
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-00
%Aladin.HpxParam    11 image color equatorial jpeg
%Aladin.Date        2017-03-27T15:44Z

%ActionName         P-CFHTLS-W-g.hpx
%Description        CFHTLS-W-g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/GALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/g
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W g
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-02
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-03-27T15:28Z

%ActionName         P-CFHTLS-W-i.hpx
%Description        CFHTLS-W-i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/IALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/i
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W i
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-04
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-03-27T15:31Z

%ActionName         P-CFHTLS-W-r.hpx
%Description        CFHTLS-W-r
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/RALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/r
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W r
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-03
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-03-27T15:34Z

%ActionName         P-CFHTLS-W-u.hpx
%Description        CFHTLS-W-u
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/UALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/u
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W u
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-01
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-03-27T15:36Z

%ActionName         P-CFHTLS-W-z.hpx
%Description        CFHTLS-W-z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/ZALLSKY
%VerboseDescr       The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter
%Copyright          (c) CFH - powered by Terapix - healpixed by CDS
%Origin             CDS
%Id                 P/CFHTLS/W/z
%Aladin.Profile     >6.1
%Copyright.Url      http://terapix.iap.fr/rubrique.php?id_rubrique=32
%SkyFraction        0.003731
%Aladin.XLabel      CFHTLS W z
%Aladin.Tree        Image/Optical/CFHTLS/WIDE
%Aladin.MenuNumber  03-04-01-05
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-03-27T15:39Z

%ActionName         P-CGPS-VGPS-CONT.hpx
%Description        Combination of the 1420 MHz continuum of the Canadian Galactic Plane Survey (CGPS) with the VLA Galactic Plane Survey (VGPS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CGPS_VGPS_CONT
%VerboseDescr       Radio continuum emission, using the Dominion Radio Astrophysical Observatory (DRAO) and the VLA telescope, at a resolution of 1'. Units: K\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/CGPS/VGPS/CONT
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.03752
%Aladin.XLabel      CGPS-VGPS CONT
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-06
%Aladin.HpxParam    4 image galactic jpeg fits
%Aladin.Date        2013-10-07T15:21Z

%ActionName         P-CGPS-VGPS.hpx
%Description        Combination of the Canadian Galactic Plane Survey (CGPS) and the VLA Galactic Plane Survey (VGPS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1457713645  2016/03/11 18:27:25
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CGPS_VGPS
%VerboseDescr       Atomic Hydrogen (integrated intensity map) emission using the Dominion Radio Astrophysical Observatory (DRAO) and the VLA telescope, at a resolution of 1'. Units: K km/s\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/CGPS/VGPS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.03571
%Aladin.XLabel      CGPS-VGPS
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.MenuNumber  06-07
%Aladin.HpxParam    4 image galactic jpeg fits
%Aladin.Date        2013-10-07T13:04Z

%ActionName         P-CHIPASS.hpx
%Description        CHIPASS 1.4 GHz Radio Continuum
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CHIPASS
%VerboseDescr       Radio continuum map of the atomic hydrogen line, of the sky south of declination +25deg. Reprocessing of archival data from the HI Parkes All-Sky Survey (HIPASS) and the HI Zone of Avoidance (HIZOA) survey. The resolution of the map is 14.4'. Units: mK\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/CHIPASS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.7159
%Aladin.XLabel      CHIPASS
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-07-08T16:43Z

%ActionName         P-CO.hpx
%Description        CO composite survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/CO
%VerboseDescr       This survey contains data from the composite CO map constructed by Dame, Hartmann and Thaddeus (2001) from 37 individual surveys of the Galaxy in the CO (1-0) line. Due to the composite nature of the map and processing used to render a uniform S/N appearance, the user is cautioned that angular resolution and sensitivity vary across the map. Survey data are limited to Galactic latitudes |b|<32 deg., with roughly half of that area containing observations.To create this file, the velocity-integrated brightness temperature map, W(CO), was obtained from the CfA Millimeter Wave Group website and then interpolated onto a HEALPix grid with Nside=512.
%Copyright          Composite map by Dame et al (2001,ApJ,547,792), - HEALPixed by LAMBDA
%Origin             CDS
%Id                 P/CO
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/foreground/fg_WCO_get.cfm
%SkyFraction        1
%Aladin.XLabel      CO composite survey
%Aladin.Tree        Image/Gas-lines/CO
%Aladin.MenuNumber  06-08-01
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2016-12-12T15:44Z

%ActionName         P-COHRS.hpx
%Description        CO High Resolution Survey (HARP/JCMT)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/COHRS
%VerboseDescr       This survey contains data from the CO High Resolution Survey (COHRS). The data we're taken in the 12CO(J=3-2) line with HARP (JCMT). The FWHM of the observations are 14". THe survey and data products are fully described in Dempsey, Thomas & Currie 2013, ApJS, 209, 8. The data cubes have been collapsed in the velocity axis between -30 and +155km/s to provide 2D integrated maps. These maps are publicly available at CADC (http://dx.doi. org/10.11570/13.0002). These 2D integrated maps were then interpolated onto a HEALPix grid with Nside=65536 at CDS
%Copyright          CANFAR
%Origin             CDS
%Id                 P/COHRS
%Aladin.Profile     >6.1
%Copyright.Url      http://www.canfar.phys.uvic.ca/canfar/
%SkyFraction        0.001495
%Aladin.XLabel      CO High Resolution Survey
%Aladin.Tree        Image/Gas-lines/CO
%Aladin.MenuNumber  06-08-02
%Aladin.HpxParam    7 image equatorial png jpeg fits
%Aladin.Date        2016-09-19T15:09Z

%ActionName         P-COMPTEL.hpx
%Description        COMPTEL 0.8-30 MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/COMPTEL
%VerboseDescr       Allsky survey (0.8-30 MeV)obtained with the imaging Gamma-ray Telescope COMPTEL aboard Nasa's Compton Gamma Ray Observatory. Units of the map are cts/s/cm^2/sr and the angular resolution is of the order of 1 degree. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/COMPTEL
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      COMPTEL 0.8-30 MeV
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-14T14:11Z

%ActionName         P-CONSTELLATIONS6.hpx
%Description        CONSTELLATIONS6
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1465811895  2016/06/13 11:58:15
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/Constellations6
%VerboseDescr       Constellation color-artworks by Kagaya studio
%Copyright          Kagaya Studio
%Origin             JAXA
%Id                 P/CONSTELLATIONS6
%Aladin.Profile     >6.1 beta
%Copyright.Url      http://www.kagayastudio.com/english/
%SkyFraction        1
%Aladin.XLabel      Artistic constellations map
%Aladin.Tree        Outreach
%Aladin.MenuNumber  ZZZZ
%Aladin.HpxParam    6 image color png
%Aladin.Date        2016-03-16T14:25Z

%ActionName         P-Callisto-Voyager-Galileo-simp-1km.hpx
%Description        Callisto Voyager-Galileo-simp-1km
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Callisto_Voyager-Galileo-simp-1km
%VerboseDescr       his global map of Callisto utilizes the best image quality and moderate resolution coverage supplied by Galileo SSI (Solid State Imaging instrument) and Voyager 1 and 2. The image processing was performed at USGS using the Integrated Software for Imagers and Spectrometers (ISIS) system. The image data was selected on the basis of overall image quality, reasonable input resolution, and availability of moderate viewing and sun angles for topography. The average input resolution was 1.0 kilometers/pixel. The resolution ranged from 60 km/pixel for gap fill up to 400 meters/pixel. The map projections are based on a sphere having a radius of 2409.3 kilometers.
%Copyright          Planetary Data System, from USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Callisto/Voyager-Galileo-simp-1km
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Callisto/Voyager-Galileo-simp-1km
%Aladin.Tree        Solar system/Jupiter/Callisto
%Aladin.HpxParam    3 image color callisto jpeg
%Aladin.Date        2018-01-21T12:42Z

%ActionName         P-Change2-moon-7m-DOM.hpx
%Description        Lunar DOM 7M
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://hips.china-vo.org/change2-moon-7m-dom
%Origin             China-VO
%Id                 P/Change2/moon/7m/DOM
%Aladin.Profile     >6.1
%SkyFraction        0.9964
%Aladin.XLabel      P/Change2/moon/7m/DOM
%Aladin.HpxParam    0 image equatorial png fits
%Aladin.Date        2019-02-03T00:05:00Z

%ActionName         P-Charon-NewHorizon-PIA19866.hpx
%Description        Charon NewHorizon PIA19866
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Charon_NewHorizon-PIA19866
%VerboseDescr       The science team of NASA's New Horizons mission has produced this global map of Pluto's largest moon, Charon. The map includes all available resolved images of the surface acquired between July 7-14, 2015, at pixel resolutions ranging from 40 kilometers (24 miles) on the anti-Pluto facing hemisphere (left and right sides of the map), to 400 meters (1,250 feet) per pixel on portions of the Pluto-facing hemisphere -- the side facing the New Horizons spacecraft when it flew past the dwarf planet -- at map center. Many additional images now stored on the spacecraft's digital data recorders are expected to be transmitted "home" in fall 2015 and these will be used to complete the global map. The map is in simple cylindrical projection, with zero longitude (the Pluto-facing direction) in the center. The Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, designed, built, and operates the New Horizons spacecraft, and manages the mission for NASA's Science Mission Directorate. The Southwest Research Institute, based in San Antonio, leads the science team, payload operations and encounter science planning. New Horizons is part of the New Frontiers Program managed by NASA's Marshall Space Flight Center in Huntsville, Alabama.
%Copyright          JPL/PhotoJournal
%Origin             CDS
%Id                 P/Charon/NewHorizon-PIA19866
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Charon/NewHorizon-PIA19866
%Aladin.Tree        Solar system/Pluto/Charon
%Aladin.HpxParam    3 image color charon jpeg
%Aladin.Date        2018-01-24T14:27Z

%ActionName         P-DECaLS-DR3-color.hpx
%Description        DECaLS DR3 color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-DECaLS-DR3-color_0.hpx availability=0
%SeeAction          P-DECaLS-DR3-color_1.hpx availability=0
%SeeAction          P-DECaLS-DR3-color_2.hpx availability=0
%SeeAction          P-DECaLS-DR3-color_3.hpx availability=9999
%VerboseDescr       The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 deg² of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18° < ? < +84° in celestial coordinates and |b||b| > 18° in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at ? < +30° using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 3 (DR3) is the third public data release of images and catalogs for the DECam Legacy Survey (DECaLS). Images from DECaLS g,r,z-band observations (NOAO survey program 0404; https://www.noao.edu/perl/abstract?2014B-0404) are included from August 2014 through March 2016. DR3 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to March 2016. In total, the optical data covers a disjoint footprint with 4300 deg² in g-band, 4600 deg² in r-band and 8100 deg² in z-band, of which 4200 deg² has been observed in all three optical filters.
%Copyright          DECam Legacy Survey
%Origin             CDS
%Id                 P/DECaLS/DR3/color
%Aladin.Profile     >6.1
%Copyright.Url      http://legacysurvey.org/
%SkyFraction        0.2275
%Aladin.XLabel      DECaLS DR3 color
%Aladin.Tree        Image/Optical/DECaLS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    11 image color equatorial jpeg
%Aladin.Date        2017-01-21T22:35Z

%ActionName         P-DECaLS-DR5-color.hpx
%Description        DECaLS DR5 color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/DECaLS/DR5/color
%VerboseDescr       The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 deg² of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18° < ? < +84° in celestial coordinates and |b||b| > 18° in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at ? < +30° using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 5 (DR5) is the fifth public data release of the Legacy Surveys. DR5 imaging is first reduced through the NOAO Community Pipeline before being processed using the Tractor. Images from DECaLS g,r,z-band observations are included from August 2014 through May 2017. DR5 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to May 2017.
%Copyright          DECam Legacy Survey
%Origin             CDS
%Id                 P/DECaLS/DR5/color
%Aladin.Profile     >6.1
%Copyright.Url      http://legacysurvey.org/
%SkyFraction        0.269
%Aladin.XLabel      DECaLS DR5 color
%Aladin.Tree        Image/Optical/DECaLS
%Aladin.HpxParam    11 image color equatorial jpeg
%Aladin.Date        2018-06-07T05:18Z

%ActionName         P-DECaLS-DR5-g.hpx
%Description        DECaLS DR5 g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/DECaLS/DR5/g
%VerboseDescr       The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 deg² of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18° < ? < +84° in celestial coordinates and |b||b| > 18° in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at ? < +30° using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 5 (DR5) is the fifth public data release of the Legacy Surveys. DR5 imaging is first reduced through the NOAO Community Pipeline before being processed using the Tractor. Images from DECaLS g,r,z-band observations are included from August 2014 through May 2017. DR5 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to May 2017.
%Copyright          DECam Legacy Survey
%Origin             CDS
%Id                 P/DECaLS/DR5/g
%Aladin.Profile     >6.1
%Copyright.Url      http://legacysurvey.org/
%SkyFraction        0.182
%Aladin.XLabel      DECaLS DR5 g
%Aladin.Tree        Image/Optical/DECaLS
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-10-17T09:17Z

%ActionName         P-DECaLS-DR5-r.hpx
%Description        DECaLS DR5 r
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/DECaLS/DR5/r
%VerboseDescr       The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 deg² of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18° < ? < +84° in celestial coordinates and |b||b| > 18° in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at ? < +30° using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 5 (DR5) is the fifth public data release of the Legacy Surveys. DR5 imaging is first reduced through the NOAO Community Pipeline before being processed using the Tractor. Images from DECaLS g,r,z-band observations are included from August 2014 through May 2017. DR5 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to May 2017.
%Copyright          DECam Legacy Survey
%Origin             CDS
%Id                 P/DECaLS/DR5/r
%Aladin.Profile     >6.1
%Copyright.Url      http://legacysurvey.org/
%SkyFraction        0.1971
%Aladin.XLabel      DECaLS DR5 r
%Aladin.Tree        Image/Optical/DECaLS
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2019-06-18T11:15Z

%ActionName         P-DECaPS-DR1-color.hpx
%Description        DECaPS DR1 color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-DECaPS-DR1-color_0.hpx availability=0
%SeeAction          P-DECaPS-DR1-color_1.hpx availability=0
%SeeAction          P-DECaPS-DR1-color_2.hpx availability=1
%VerboseDescr       The DECam Plane Survey is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera at Cerro Tololo. The survey is designed to reach past the mainsequence turn-off at the distance of the Galactic center through a reddening E(B - V ) of 1.5 mag.  Typical single-exposure depths are 23.7, 22.8, 22.3, 21.9, and 21.0 mag in the grizY bands, with seeing around 100. The footprint covers the Galactic plane with |b| <= 4 degrees , 5 degrees > l > 120 degrees
%Copyright          DECaM Plane Survey / NOAO
%Origin             CDS
%Id                 P/DECaPS/DR1/color
%Aladin.Profile     >6.1
%Copyright.Url      http://decaps.skymaps.info/
%SkyFraction        0.03543
%Aladin.XLabel      DECam Plane Survey DR1 color (g, r, z bands)
%Aladin.Tree        Image/Optical/DECaPS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    11 image color equatorial png jpeg
%Aladin.Date        2018-01-31T09:34Z

%ActionName         P-DECaPS-DR1-g.hpx
%Description        DECaPS DR1 g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/DECaPS/DR1/g
%VerboseDescr       The DECam Plane Survey is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera at Cerro Tololo. The survey is designed to reach past the mainsequence turn-off at the distance of the Galactic center through a reddening E(B ? V ) of 1.5 mag.  Typical single-exposure depths are 23.7, 22.8, 22.3, 21.9, and 21.0 mag in the grizY bands, with seeing around 100. The footprint covers the Galactic plane with |b| <= 4? , 5? > l > ?120?
%Copyright          DECaM Plane Survey / NOAO
%Origin             CDS
%Id                 P/DECaPS/DR1/g
%Aladin.Profile     >6.1
%Copyright.Url      http://decaps.skymaps.info/
%SkyFraction        0.0351
%Aladin.XLabel      DECam Plane Survey DR1 g band
%Aladin.Tree        Image/Optical/DECaPS
%Aladin.HpxParam    11 image equatorial png jpeg fits
%Aladin.Date        2018-01-19T03:17Z

%ActionName         P-DES-DR1-LIneA-color.hpx
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%VerboseDescr       The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars.
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%VerboseDescr       The dard Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed understanding the accelerating explansion rate of the universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars.
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%VerboseDescr       The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars.
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%VerboseDescr       The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars.
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%VerboseDescr       The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars.
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%ActionName         P-DIRBE-10.hpx
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%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 2 -2.2 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
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%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 4 - 4.9 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
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%ActionName         P-DIRBE-ZSMA5.hpx
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%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DIRBE_ZSMA_5
%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 5 - 12 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
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%ActionName         P-DIRBE-ZSMA6.hpx
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%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DIRBE_ZSMA_6
%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 6 - 25 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
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%ActionName         P-DIRBE-ZSMA7.hpx
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%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 7 - 60 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
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%ActionName         P-DIRBE-ZSMA8.hpx
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%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DIRBE_ZSMA_8
%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 8 - 100 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DIRBE/ZSMA8
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      DIRBE ZSMA band 8 - 100um
%Aladin.Tree        Image/Infrared/DIRBE/ZSMA
%Aladin.MenuNumber  04-01-Z01-08
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-09-02T13:00Z

%ActionName         P-DIRBE-ZSMA9.hpx
%Description        DIRBE ZSMA BAND 9 - 140 mic
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DIRBE_ZSMA_9
%VerboseDescr       All-sky survey performed with the COBE/DIRBE instrument (Band 9 - 140 microns) at the 1deg resolution. Zodi-subtracted map. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DIRBE/ZSMA9
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      DIRBE ZSMA band 9 - 140um
%Aladin.Tree        Image/Infrared/DIRBE/ZSMA
%Aladin.MenuNumber  04-01-Z01-09
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-09-02T13:02Z

%ActionName         P-DM-I-345-gaia2.hpx
%Description        Density map for Gaia DR2 (I/345/gaia2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/hips-density-map
%Origin             CDS
%Id                 P/DM/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    4 image equatorial jpeg fits
%Aladin.Date        2018-04-17T10:36Z

%ActionName         P-DM-flux-Bp-I-345-gaia2.hpx
%Description        Bp flux map for table I/345/gaia2 (Gaia DR2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/Bp-flux-map
%Origin             CDS
%Id                 P/DM/flux-Bp/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/flux-Bp/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    4 image equatorial jpeg fits
%Aladin.Date        2018-04-17T08:03Z

%ActionName         P-DM-flux-G-I-345-gaia2.hpx
%Description        G flux map for table I/345/gaia2 (Gaia DR2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/G-flux-map
%Origin             CDS
%Id                 P/DM/flux-G/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/flux-G/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    4 image equatorial jpeg fits
%Aladin.Date        2018-04-17T07:08Z

%ActionName         P-DM-flux-Rp-I-345-gaia2.hpx
%Description        Rp flux map for table I/345/gaia2 (Gaia DR2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/Rp-flux-map
%Origin             CDS
%Id                 P/DM/flux-Rp/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/flux-Rp/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    4 image equatorial jpeg fits
%Aladin.Date        2018-04-17T08:18Z

%ActionName         P-DM-flux-color-Rp-G-Bp-I-345-gaia2.hpx
%Description        Color flux map for I/345/gaia2 (Gaia DR2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/color-Rp-G-Bp-flux-map
%Origin             CDS
%Id                 P/DM/flux-color-Rp-G-Bp/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/flux-color-Rp-G-Bp/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    4 image color equatorial jpeg
%Aladin.Date        2018-04-19T12:46Z

%ActionName         P-DM-radial-velocity-I-345-gaia2.hpx
%Description        Radial velocity map for I/345/gaia2 (Gaia DR2)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ancillary/GaiaDR2/radial-velocity-map
%Origin             CDS
%Id                 P/DM/radial-velocity/I/345/gaia2
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/radial-velocity/I/345/gaia2
%Aladin.Tree        Ancillary/GaiaDR2
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2018-04-26T22:03Z

%ActionName         P-DM-simbad-biblio-allObjects.hpx
%Description        Simbad heatmap - all objects
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/allObjects
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/allObjects
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/allObjects
%Aladin.Tree        Ancillary/Simbad bibliography
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:23Z

%ActionName         P-DM-simbad-biblio-otypes-Galaxy.hpx
%Description        Simbad heatmap - Galaxy
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Galaxy
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Galaxy
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Galaxy
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:26Z

%ActionName         P-DM-simbad-biblio-otypes-HII.hpx
%Description        Simbad heatmap - HII
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/HII
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/HII
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/HII
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:24Z

%ActionName         P-DM-simbad-biblio-otypes-Infrared.hpx
%Description        Simbad heatmap - Infrared
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Infrared
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Infrared
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Infrared
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:26Z

%ActionName         P-DM-simbad-biblio-otypes-Nebula.hpx
%Description        Simbad heatmap - Nebula
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Nebula
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Nebula
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Nebula
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:25Z

%ActionName         P-DM-simbad-biblio-otypes-Other.hpx
%Description        Simbad heatmap - Other
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Other
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Other
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Other
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:25Z

%ActionName         P-DM-simbad-biblio-otypes-Radio.hpx
%Description        Simbad heatmap - Radio
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Radio
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Radio
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Radio
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:25Z

%ActionName         P-DM-simbad-biblio-otypes-Star.hpx
%Description        Simbad heatmap - Star
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/Star
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/Star
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/Star
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:24Z

%ActionName         P-DM-simbad-biblio-otypes-UV.hpx
%Description        Simbad heatmap - UV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/UV
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/UV
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/UV
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:23Z

%ActionName         P-DM-simbad-biblio-otypes-X.hpx
%Description        Simbad heatmap - X
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/X
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/otypes/X
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/otypes/X
%Aladin.Tree        Ancillary/Simbad bibliography/By object types
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:24Z

%ActionName         P-DM-simbad-biblio-pub-dates-1850-1900.hpx
%Description        Simbad heatmap - 1850-1900
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1850-1900
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1850-1900
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1850-1900
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:26Z

%ActionName         P-DM-simbad-biblio-pub-dates-1900-1910.hpx
%Description        Simbad heatmap - 1900-1910
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1900-1910
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1900-1910
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1900-1910
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:27Z

%ActionName         P-DM-simbad-biblio-pub-dates-1910-1920.hpx
%Description        Simbad heatmap - 1910-1920
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1910-1920
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1910-1920
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1910-1920
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:27Z

%ActionName         P-DM-simbad-biblio-pub-dates-1920-1930.hpx
%Description        Simbad heatmap - 1920-1930
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1920-1930
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1920-1930
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1920-1930
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:27Z

%ActionName         P-DM-simbad-biblio-pub-dates-1930-1940.hpx
%Description        Simbad heatmap - 1930-1940
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1930-1940
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1930-1940
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1930-1940
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:27Z

%ActionName         P-DM-simbad-biblio-pub-dates-1940-1945.hpx
%Description        Simbad heatmap - 1940-1945
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1940-1945
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1940-1945
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1940-1945
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:28Z

%ActionName         P-DM-simbad-biblio-pub-dates-1945-1950.hpx
%Description        Simbad heatmap - 1945-1950
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1945-1950
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1945-1950
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1945-1950
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:28Z

%ActionName         P-DM-simbad-biblio-pub-dates-1950-1955.hpx
%Description        Simbad heatmap - 1950-1955
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1950-1955
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1950-1955
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1950-1955
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:28Z

%ActionName         P-DM-simbad-biblio-pub-dates-1955-1960.hpx
%Description        Simbad heatmap - 1955-1960
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1955-1960
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1955-1960
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1955-1960
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:29Z

%ActionName         P-DM-simbad-biblio-pub-dates-1960-1965.hpx
%Description        Simbad heatmap - 1960-1965
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1960-1965
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1960-1965
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1960-1965
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:29Z

%ActionName         P-DM-simbad-biblio-pub-dates-1965-1970.hpx
%Description        Simbad heatmap - 1965-1970
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1965-1970
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1965-1970
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1965-1970
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:29Z

%ActionName         P-DM-simbad-biblio-pub-dates-1970-1975.hpx
%Description        Simbad heatmap - 1970-1975
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1970-1975
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1970-1975
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1970-1975
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:29Z

%ActionName         P-DM-simbad-biblio-pub-dates-1975-1980.hpx
%Description        Simbad heatmap - 1975-1980
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1975-1980
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1975-1980
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1975-1980
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:30Z

%ActionName         P-DM-simbad-biblio-pub-dates-1980-1985.hpx
%Description        Simbad heatmap - 1980-1985
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1980-1985
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1980-1985
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1980-1985
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:30Z

%ActionName         P-DM-simbad-biblio-pub-dates-1985-1990.hpx
%Description        Simbad heatmap - 1985-1990
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1985-1990
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1985-1990
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1985-1990
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:30Z

%ActionName         P-DM-simbad-biblio-pub-dates-1991.hpx
%Description        Simbad heatmap - 1991
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1991
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1991
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1991
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:31Z

%ActionName         P-DM-simbad-biblio-pub-dates-1992.hpx
%Description        Simbad heatmap - 1992
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1992
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1992
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1992
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:31Z

%ActionName         P-DM-simbad-biblio-pub-dates-1993.hpx
%Description        Simbad heatmap - 1993
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1993
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1993
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1993
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:31Z

%ActionName         P-DM-simbad-biblio-pub-dates-1994.hpx
%Description        Simbad heatmap - 1994
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1994
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1994
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1994
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:32Z

%ActionName         P-DM-simbad-biblio-pub-dates-1995.hpx
%Description        Simbad heatmap - 1995
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1995
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1995
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1995
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:32Z

%ActionName         P-DM-simbad-biblio-pub-dates-1996.hpx
%Description        Simbad heatmap - 1996
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1996
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1996
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1996
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:32Z

%ActionName         P-DM-simbad-biblio-pub-dates-1997.hpx
%Description        Simbad heatmap - 1997
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1997
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1997
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1997
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:33Z

%ActionName         P-DM-simbad-biblio-pub-dates-1998.hpx
%Description        Simbad heatmap - 1998
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1998
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1998
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1998
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:33Z

%ActionName         P-DM-simbad-biblio-pub-dates-1999.hpx
%Description        Simbad heatmap - 1999
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/1999
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/1999
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/1999
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:33Z

%ActionName         P-DM-simbad-biblio-pub-dates-2000.hpx
%Description        Simbad heatmap - 2000
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2000
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2000
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2000
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:34Z

%ActionName         P-DM-simbad-biblio-pub-dates-2001.hpx
%Description        Simbad heatmap - 2001
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2001
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2001
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2001
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:34Z

%ActionName         P-DM-simbad-biblio-pub-dates-2002.hpx
%Description        Simbad heatmap - 2002
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2002
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2002
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2002
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:34Z

%ActionName         P-DM-simbad-biblio-pub-dates-2003.hpx
%Description        Simbad heatmap - 2003
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2003
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2003
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2003
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:35Z

%ActionName         P-DM-simbad-biblio-pub-dates-2004.hpx
%Description        Simbad heatmap - 2004
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2004
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2004
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2004
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:35Z

%ActionName         P-DM-simbad-biblio-pub-dates-2005.hpx
%Description        Simbad heatmap - 2005
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2005
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2005
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2005
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:35Z

%ActionName         P-DM-simbad-biblio-pub-dates-2006.hpx
%Description        Simbad heatmap - 2006
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2006
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2006
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2006
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:36Z

%ActionName         P-DM-simbad-biblio-pub-dates-2007.hpx
%Description        Simbad heatmap - 2007
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2007
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2007
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2007
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:36Z

%ActionName         P-DM-simbad-biblio-pub-dates-2008.hpx
%Description        Simbad heatmap - 2008
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2008
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2008
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2008
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:36Z

%ActionName         P-DM-simbad-biblio-pub-dates-2009.hpx
%Description        Simbad heatmap - 2009
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2009
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2009
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2009
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:37Z

%ActionName         P-DM-simbad-biblio-pub-dates-2010.hpx
%Description        Simbad heatmap - 2010
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2010
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2010
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2010
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:37Z

%ActionName         P-DM-simbad-biblio-pub-dates-2011.hpx
%Description        Simbad heatmap - 2011
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2011
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2011
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2011
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:38Z

%ActionName         P-DM-simbad-biblio-pub-dates-2012.hpx
%Description        Simbad heatmap - 2012
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2012
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2012
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2012
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:38Z

%ActionName         P-DM-simbad-biblio-pub-dates-2013.hpx
%Description        Simbad heatmap - 2013
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2013
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2013
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2013
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:38Z

%ActionName         P-DM-simbad-biblio-pub-dates-2014.hpx
%Description        Simbad heatmap - 2014
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2014
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2014
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2014
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:39Z

%ActionName         P-DM-simbad-biblio-pub-dates-2015.hpx
%Description        Simbad heatmap - 2015
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2015
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2015
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2015
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:39Z

%ActionName         P-DM-simbad-biblio-pub-dates-2016.hpx
%Description        Simbad heatmap - 2016
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2016
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2016
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2016
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:39Z

%ActionName         P-DM-simbad-biblio-pub-dates-2017.hpx
%Description        Simbad heatmap - 2017
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2017
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2017
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2017
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:39Z

%ActionName         P-DM-simbad-biblio-pub-dates-2018.hpx
%Description        Simbad heatmap - 2018
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2018
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2018
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2018
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:40Z

%ActionName         P-DM-simbad-biblio-pub-dates-2019.hpx
%Description        Simbad heatmap - 2019
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/2019
%Copyright          © Université de Strasbourg - CNRS. All rights reserved
%Origin             CDS
%Id                 P/DM/simbad-biblio/pub-dates/2019
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/DM/simbad-biblio/pub-dates/2019
%Aladin.Tree        Ancillary/Simbad bibliography/By publication dates
%Aladin.HpxParam    3 image equatorial fits png
%Aladin.Date        2019-03-25T10:40Z

%ActionName         P-DRAO-22MHz.hpx
%Description        DRAO 22 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DRAO_22MHz
%VerboseDescr       Northern sky survey at 22.25 MHz using the radio telescope at Dominion Radio Astrophysical Observatory (DRAO); The resolution of the telescope is 1.1degx1.7degsecant(zenith angle). Units: KTB.\nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DRAO/22MHz
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.7283
%Aladin.XLabel      DRAO 22MHz
%Aladin.Tree        Image/Radio/DRAO
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-09-01T15:04Z

%ActionName         P-DRAO-VillaElisa-21cm-POLQ.hpx
%Description        DRAO-VillaElisa 21cm POLQ
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DRAO-VillaElisa_21cm_POLQ
%VerboseDescr       21cm All-sky polarization survey (Stokes Q) using the combination of the 26-m DRAO and 30-m Villa Elisa data, at an angular resolution of 36?. Units: mKTB.\nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DRAO-VillaElisa/21cm/POLQ
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      DRAO-VillaElisa 21cm POLQ
%Aladin.Tree        Image/Radio/DRAO
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-13T13:32Z

%ActionName         P-DRAO-VillaElisa-21cm-POLU.hpx
%Description        DRAO-VillaElisa 21cm POLU
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/DRAO-VillaElisa_21cm_POLU
%VerboseDescr       21cm All-sky polarization survey (Stokes U) using the combination of the 26-m DRAO and 30-m Villa Elisa data, at an angular resolution of 36?. Units: mKTB.\nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DRAO-VillaElisa/21cm/POLU
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      DRAO-VillaElisa 21cm POLU
%Aladin.Tree        Image/Radio/DRAO
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-13T14:15Z

%ActionName         P-DSS2-NIR.hpx
%Description        DSS2 NIR (XI+IS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/DSS/DSS2-NIR
%VerboseDescr       The Catalogs and Surveys Group of the Space Telescope Science Institute has digitized the photographic Sky survey plates from the Palomar and  UK Schmidt telescopes to produce the "Digitized Sky Survey"(DSS). Each plate  covers 6.5 x 6.5 degrees of the sky and have been digitized using a modified  PDS microdensitometer. The DSS NIT HiPS is a combination of DSS2-XI and DSS2-IS. DSS2-XI north is the digitalization of the POSS-II N (1987-2002 - filter: IV-N +RG9) from Caltech, DSS2-IS south is the digitalization of the SERC-IS (1990-2002 - filter: IV-N +RG175). The all-sky HEALPix resampling has been done by the CDS with the help of CADC.
%Copyright          Digitized Sky Survey - STScI/NASA, Healpixed by CDS
%Origin             CDS
%Id                 P/DSS2/NIR
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.stsci.edu/dss/copyright.html
%SkyFraction        0.9943
%Aladin.XLabel      DSS2 NIR (XI+IS)
%Aladin.Tree        Image/Optical/DSS
%Aladin.MenuNumber  03-01-03a
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2016-12-13T15:18Z

%ActionName         P-DSS2-blue.hpx
%Description        DSS2 Blue (XJ+S)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-DSS2-blue_0.hpx availability=0
%SeeAction          P-DSS2-blue_1.hpx availability=0
%SeeAction          P-DSS2-blue_2.hpx availability=0
%VerboseDescr       The Catalogs and Surveys Group of the Space Telescope Science Institute has digitized the photographic Sky survey plates from the Palomar and  UK Schmidt telescopes to produce the "Digitized Sky Survey"(DSS). Each plate  covers 6.5 x 6.5 degrees of the sky and have been\ndigitized using a modified  PDS microdensitometer. The DSS blue HiPS is a combination of DSS2-XJ and DSS2-S. DSS2-XJ north is the digitalization of the POSS-II J (1987-1998 - 0.491um) from Caltech,DSS2-S south is the digitalization of the SERC-J (1975-1987 - 0.468um) and SERC-EJ (1979-1988 - 0.468um) from ROE.The all-sky HEALPix resampling has been done by the CDS with the help of CADC.
%Copyright          Digitized Sky Survey - STScI/NASA, Healpixed by CDS
%Origin             CDS
%Id                 P/DSS2/blue
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.stsci.edu/dss/copyright.html
%SkyFraction        0.9956
%Aladin.XLabel      DSS2 Blue (XJ+S)
%Aladin.Tree        Image/Optical/DSS
%Aladin.MenuNumber  03-01-03 lite
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2015-02-07T11:42Z

%ActionName         P-DSS2-color.hpx
%Description        DSS colored
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-DSS2-color_0.hpx availability=0
%SeeAction          P-DSS2-color_1.hpx availability=10
%SeeAction          P-DSS2-color_2.hpx availability=0
%SeeAction          P-DSS2-color_3.hpx availability=0
%SeeAction          P-DSS2-color_4.hpx availability=9999
%SeeAction          P-DSS2-color_5.hpx availability=11
%SeeAction          P-DSS2-color_6.hpx availability=1055
%SeeAction          P-DSS2-color_7.hpx availability=14
%VerboseDescr       Color composition generated by CDS. This HiPS survey is based on 2 others HiPS surveys, respectively DSS2-red and DSS2-blue HiPS, both of them directly generated from original scanned plates downloaded from STScI site. The red component has been built from POSS-II F, AAO-SES,SR and SERC-ER plates. The blue component has been build from POSS-II J and SERC-J,EJ. The green component is based on the mean of other components. Three missing plates from red survey (253, 260, 359) has been replaced by pixels from the DSSColor STScI jpeg survey. The 11 missing blue plates (mainly in galactic plane) have not been replaced (only red component).
%Copyright          Digitized Sky Survey - STScI/NASA, Colored & Healpixed by CDS
%Origin             CDS
%Id                 P/DSS2/color
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.stsci.edu/dss/copyright.html
%SkyFraction        1
%Aladin.XLabel      DSS colored
%Aladin.Tree        Image/Optical/DSS
%Aladin.MenuNumber  03-00 lite
%Aladin.HpxParam    9 image color equatorial jpeg
%Aladin.Date        2015-05-11T08:45Z

%ActionName         P-DSS2-red.hpx
%Description        DSS2 Red (F+R)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-DSS2-red_0.hpx availability=0
%SeeAction          P-DSS2-red_1.hpx availability=11
%SeeAction          P-DSS2-red_2.hpx availability=0
%SeeAction          P-DSS2-red_3.hpx availability=0
%SeeAction          P-DSS2-red_4.hpx availability=1055
%SeeAction          P-DSS2-red_5.hpx availability=14
%VerboseDescr       The Catalogs and Surveys Group of the Space Telescope Science  Institute has digitized the photographic Sky survey plates from the Palomar and UK Schmidt telescopes to produce the "Digitized Sky Survey" (DSS). Each plate covers 6.5 x 6.5 degrees of the sky and have been digitized using a modified PDS microdensitometer.\nDSS2F north is the digitalization of the POSS2/UKSTU Red survey (0.658um)\nDSS2R south is the digitalization of the AAO Red survey (0.64um)\nThe all-sky HEALPix resampling has been done by the CDS
%Copyright          Digitized Sky Survey - STScI/NASA, Healpixed by CDS
%Origin             CDS
%Id                 P/DSS2/red
%Aladin.Profile     >6.1
%Copyright.Url      http://archive.stsci.edu/dss/copyright.html
%SkyFraction        1
%Aladin.XLabel      DSS2 Red (F+R)
%Aladin.Tree        Image/Optical/DSS
%Aladin.MenuNumber  03-01-02 lite
%Aladin.HpxParam    9 image equatorial jpeg fits
%Aladin.Date        2014-10-24T14:57Z

%ActionName         P-DWINGELOO-820MHz.hpx
%Description        Dwingeloo 820MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488879804  2017/03/07 11:43:24
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Dwingeloo_820MHz
%VerboseDescr       Continuum radiation at 820 MHz using the Dwingeloo telescope, with an effective resolution of 1.2 degree. Units: K\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/DWINGELOO/820MHz
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.5723
%Aladin.XLabel      DWINGELOO 820MHz
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-02-09T13:51Z

%ActionName         P-Dione-Cassini-PIA12577.hpx
%Description        Dione Cassini PIA12577
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Dione_Cassini-PIA12577
%VerboseDescr       This global map of Saturn's moon Dione was created using images taken during flybys by NASA's Cassini spacecraft. Images from NASA's Voyager mission fill the gaps in Cassini's coverage. The map is a simple cylindrical (equidistant) projection and has a scale of 153 meters (500 feet) per pixel at the equator. The resolution of the map is 64 pixels per degree. The mean radius of Dione used for projection of this map is 563 kilometers (350 miles). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate in Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.
%Copyright          JPL/PhotoJournal
%Origin             CDS
%Id                 P/Dione/Cassini-PIA12577
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Dione/Cassini-PIA12577
%Aladin.Tree        Solar system/Saturn/Dione
%Aladin.HpxParam    3 image color dione jpeg
%Aladin.Date        2018-01-24T13:47Z

%ActionName         P-EBHIS.hpx
%Description        EBHIS 21cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EBHIS
%VerboseDescr       Effelsberg-Bonn HI Survey (EBHIS) covering the northern sky (Dec>-5°) of the Milky-Way and the local volume out to a redshift of z=0.07. The angular resolution is 10.8?. Units: cm-2\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EBHIS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.5468
%Aladin.XLabel      EBHIS 21cm
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2018-03-05T09:12Z

%ActionName         P-EFFELSBERG+EMLS-21cm-.hpx
%Description        EFFELSBERG+EMLS 21cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG+EMLS_21cm
%VerboseDescr       Combination of the Galactic plane and medium latitude surveys with the Effelsberg 100m telescope at 1408 MHz (only source component), at a resolution of 9.4?. Units:mKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG+EMLS/21cm/
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.07493
%Aladin.XLabel      EFFELSBERG+EMLS 21cm
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-23T12:58Z

%ActionName         P-EFFELSBERG+EMLS-21cm-back.hpx
%Description        EFFELSBERG+EMLS 21cm background
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG+EMLS_21cm_back
%VerboseDescr       Combination of the Galactic plane and medium latitude surveys with the Effelsberg 100m telescope at 1408 MHz (background component), at a resolution of 9.4?. Units:mKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG+EMLS/21cm/back
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.07916
%Aladin.XLabel      EFFELSBERG+EMLS 21cm back
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-23T13:36Z

%ActionName         P-EFFELSBERG-11cm-POLQ.hpx
%Description        Effelsberg 11cm POLQ
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_11cm_POLQ
%VerboseDescr       Polarization survey (Stokes Q) of the Galactic plane carried out with the Effelsberg 100-m telescope at 2695 MHz, at the 4.3? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/11cm/POLQ
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.02846
%Aladin.XLabel      EFFELSBERG 11cm POLQ
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-12-07T14:29Z

%ActionName         P-EFFELSBERG-11cm-POLU.hpx
%Description        Effelsberg 11cm POLU
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_11cm_POLU
%VerboseDescr       Polarization survey (Stokes U) of the Galactic plane carried out with the Effelsberg 100-m telescope at 2695 MHz, at the 4.3? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/11cm/POLU
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.02846
%Aladin.XLabel      EFFELSBERG 11cm POLU
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-12-07T14:30Z

%ActionName         P-EFFELSBERG-11cm-back.hpx
%Description        Effelsberg 11cm background
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_11cm_back
%VerboseDescr       Galactic plane survey at 2695 MHz (background component) at the 4.3? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/11cm/back
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.01985
%Aladin.XLabel      EFFELSBERG 11cm back
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-22T14:22Z

%ActionName         P-EFFELSBERG-11cm.hpx
%Description        Effelsberg 11cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_11cm
%VerboseDescr       Galactic plane survey at 2695 MHz (only source component) at the 4.3? resolution. Units: mKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/11cm
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.06151
%Aladin.XLabel      EFFELSBERG 11cm
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-22T13:56Z

%ActionName         P-EFFELSBERG-21cm-POLQ.hpx
%Description        Effelsberg 21cm POLQ
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_21cm_POLQ
%VerboseDescr       Polarization survey (Stokes Q) at medium Galactic latitudes carried out with the Effelsberg 100-m telescope at 1.4 GHz, at the 9.4? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/21cm/POLQ
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.04883
%Aladin.XLabel      EFFELSBERG 21cm POLQ
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-12-05T13:36Z

%ActionName         P-EFFELSBERG-21cm-POLU.hpx
%Description        Effelsberg 21cm POLU
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_21cm_POLU
%VerboseDescr       Polarization survey (Stokes U) at medium Galactic latitudes carried out with the Effelsberg 100-m telescope at 1.4 GHz, at the 9.4? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/21cm/POLU
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.04883
%Aladin.XLabel      EFFELSBERG 21cm POLU
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-12-07T14:31Z

%ActionName         P-EFFELSBERG-21cm-back.hpx
%Description        Effelsberg 21cm background
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_21cm_back
%VerboseDescr       Galactic plane survey at 1408 MHz (background component) at the 9.4? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/21cm/back
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05175
%Aladin.XLabel      EFFELSBERG 21cm back
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-18T16:27Z

%ActionName         P-EFFELSBERG-21cm.hpx
%Description        Effelsberg 21cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/EFFELSBERG_21cm
%VerboseDescr       Galactic plane survey at 1408 MHz (only source component) at the 9.4? resolution. Units: mKTB\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/EFFELSBERG/21cm
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05141
%Aladin.XLabel      EFFELSBERG 21cm
%Aladin.Tree        Image/Radio/EFFELSBERG
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-22T14:08Z

%ActionName         P-EGRET-Dif-100-150.hpx
%Description        EGRET Dif 100-150MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_100-150
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/100-150
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 100-150MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-04
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T14:11Z

%ActionName         P-EGRET-Dif-1000-2000.hpx
%Description        EGRET Dif 1000-2000MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_1000-2000
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/1000-2000
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 1000-2000MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-08
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:21Z

%ActionName         P-EGRET-Dif-150-300.hpx
%Description        EGRET Dif 150-300MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_150-300
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/150-300
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 150-300MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-05
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:24Z

%ActionName         P-EGRET-Dif-2000-4000.hpx
%Description        EGRET Dif 2000-4000MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_2000-4000
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/2000-4000
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 2000-4000MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-09
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:27Z

%ActionName         P-EGRET-Dif-30-50.hpx
%Description        EGRET Dif 30-50MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_30-50
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/30-50
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 30-50MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-01
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:28Z

%ActionName         P-EGRET-Dif-300-500.hpx
%Description        EGRET Dif 300-500MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_300-500
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/300-500
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 300-500MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-06
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:30Z

%ActionName         P-EGRET-Dif-4000-10000.hpx
%Description        EGRET Dif 4000-10000MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_4000-10000
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/4000-10000
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 4000-10000MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-10
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:32Z

%ActionName         P-EGRET-Dif-50-70.hpx
%Description        EGRET Dif 50-70MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_50-70
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/50-70
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 50-70MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-02
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:33Z

%ActionName         P-EGRET-Dif-500-1000.hpx
%Description        EGRET Dif 500-1000MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_500-1000
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/500-1000
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 500-1000MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-07
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:35Z

%ActionName         P-EGRET-Dif-70-100.hpx
%Description        EGRET Dif 70-100MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_70-100
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/Dif/70-100
%Aladin.Profile     >6.1
%Copyright.Url      ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html
%SkyFraction        1
%Aladin.XLabel      Diffuse Gamma-ray EGRET maps - 70-100MeV
%Aladin.Tree        Image/Gamma-ray/EGRET/Diffuse
%Aladin.MenuNumber  00-02-01-03
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:37Z

%ActionName         P-EGRET-inf100.hpx
%Description        EGRET inf 100MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-inf100
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS	Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/inf100
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      Gamma-ray EGRET maps - inf 100MeV
%Aladin.Tree        Image/Gamma-ray/EGRET
%Aladin.MenuNumber  00-02-00a
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:38Z

%ActionName         P-EGRET-sup100.hpx
%Description        EGRET sup 100MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/EGRET/EGRET-sup100
%VerboseDescr       This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS	Compton Gamma Ray Observatory (CGRO)
%Origin             CDS
%Id                 P/EGRET/sup100
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      Gamma-ray EGRET maps - sup 100MeV
%Aladin.Tree        Image/Gamma-ray/EGRET
%Aladin.MenuNumber  00-02-00b
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-09-20T15:40Z

%ActionName         P-Earth-BlueMarble.hpx
%Description        Blue Marble Next Generation w/ Topography and Bathymetry
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Earth_BlueMarble
%VerboseDescr       Blue Marble: Next Generation offers greater spatial detail of the surface and spans a longer data collection period than the original. The original Blue Marble was a composite of four months of MODIS observations with a spatial resolution (level of detail) of 1 square kilometer per pixel. Blue Marble: Next Generation offers a years worth of monthly composites at a spatial resolution of 500 meters. These monthly images reveal seasonal changes to the land surface: the green-up and dying-back of vegetation in temperate regions such as North America and Europe, dry and wet seasons in the tropics, and advancing and retreating Northern Hemisphere snow cover. From a computer processing standpoint, the major improvement is the development of a new technique for allowing the computer to automatically recognize and remove cloud-contaminated or otherwise bad data?a process that was previously done manually. Credit: Blue Marble: Next Generation was produced by Reto St?ckli, NASA Earth Observatory (NASA Goddard Space Flight Center)
%Copyright          NASA's Earth Observatory
%Origin             CDS
%Id                 P/Earth/BlueMarble
%Aladin.Profile     >6.1 beta
%Copyright.Url      https://earthobservatory.nasa.gov/Features/BlueMarble/
%SkyFraction        1
%Aladin.XLabel      P/Earth/BlueMarble
%Aladin.Tree        Solar system/Earth
%Aladin.HpxParam    5 image color earth jpeg
%Aladin.Date        2018-01-21T16:50Z

%ActionName         P-Enceladus-Cassini-110m.hpx
%Description        Enceladus Cassini 110m (PIA 12564)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Enceladus_Cassini-110m
%VerboseDescr       The Cassini Equinox Mission is a joint United States and European endeavor. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.
%Copyright          USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Enceladus/Cassini-110m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Enceladus/Cassini-110m
%Aladin.Tree        Solar system/Saturn/Enceladus
%Aladin.HpxParam    3 image color enceladus jpeg
%Aladin.Date        2018-01-24T11:45Z

%ActionName         P-Europa-Voyager-GalileoSSI-500m.hpx
%Description        Europa Voyager-GalileoSSI-500m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Europa_Voyager-GalileoSSI-500m
%VerboseDescr       This global map base of Europa utilizes the best image quality and moderate resolution coverage supplied by the Galileo SSI (Solid-State Imaging) instrument and Voyager 1 and 2. The image processing was performed at the USGS Astrogeology Science Center using the Integrated Software for Imagers and Spectrometers (ISIS2) system. The image data was selected on the basis of overall image quality, reasonable input resolution (from 20 km/pixel for gap fill to as high as 200 meters/pixel), and availability of moderate viewing and sun angles for topography. The map projections are based on a sphere having a radius of 1,562.09 kilometers.
%Copyright          Public domain
%Origin             CDS
%Id                 P/Europa/Voyager-GalileoSSI-500m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Europa/Voyager-GalileoSSI-500m
%Aladin.Tree        Solar system/Jupiter/Europa
%Aladin.HpxParam    3 image color europa jpeg
%Aladin.Date        2018-01-21T12:48Z

%ActionName         P-Fermi-3.hpx
%Description        Fermi 300-1000MeV HEALPix survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/Fermi/300-1000MeV
%VerboseDescr       Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS
%Origin             CDS
%Id                 P/Fermi/3
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        1
%Aladin.XLabel      Fermi3 300-1000MeV
%Aladin.Tree        Image/Gamma-ray
%Aladin.MenuNumber  00-01-04
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-11-30T15:35Z

%ActionName         P-Fermi-4.hpx
%Description        Fermi 1-3GeV HEALPix survey.
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/Fermi/1-3GeV
%VerboseDescr       Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS
%Origin             CDS
%Id                 P/Fermi/4
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        1
%Aladin.XLabel      Fermi4 1-3GeV
%Aladin.Tree        Image/Gamma-ray
%Aladin.MenuNumber  00-01-03
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-11-30T15:24Z

%ActionName         P-Fermi-5.hpx
%Description        Fermi 3-300GeV HEALPix survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/Fermi/3-300GeV
%VerboseDescr       Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS
%Origin             CDS
%Id                 P/Fermi/5
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        1
%Aladin.XLabel      Fermi5 3-300GeV
%Aladin.Tree        Image/Gamma-ray
%Aladin.MenuNumber  00-01-02
%Aladin.HpxParam    3 image equatorial jpeg fits
%Aladin.Date        2016-11-30T15:50Z

%ActionName         P-Fermi-Band1.hpx
%Description        Fermi-LAT 30-100 MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Fermi_Band1
%VerboseDescr       Fermi-LAT all-sky survey in Band 1 (30-100 MeV), at an angular resolution of 3 degrees. Units are cnts/s/cm^2/sr. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Fermi/Band1
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Fermi-LAT 30-100 MeV
%Aladin.Tree        Image/Gamma-ray/Fermi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-11T12:35Z

%ActionName         P-Fermi-Band2.hpx
%Description        Fermi-LAT 100-300 MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Fermi_Band2
%VerboseDescr       Fermi-LAT all-sky survey in Band 2 (100-300 MeV), at an angular resolution of 2 degrees. Units are cnts/s/cm^2/sr. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Fermi/Band2
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Fermi-LAT 100-300 MeV
%Aladin.Tree        Image/Gamma-ray/Fermi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-11T12:37Z

%ActionName         P-Fermi-Band3.hpx
%Description        Fermi-LAT 300-1000 MeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Fermi_Band3
%VerboseDescr       Fermi-LAT all-sky survey in Band 3 (300-1000 MeV), at an angular resolution of 1 degree. Units are cnts/s/cm^2/sr. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Fermi/Band3
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Fermi-LAT 300-1000 MeV
%Aladin.Tree        Image/Gamma-ray/Fermi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-11T12:39Z

%ActionName         P-Fermi-Band4.hpx
%Description        Fermi-LAT 1-3 GeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Fermi_Band4
%VerboseDescr       Fermi-LAT all-sky survey in Band 4 (1-3 GeV), at an angular resolution of 0.4 degrees. Units are cnts/s/cm^2/sr. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Fermi/Band4
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Fermi-LAT 1-3 GeV
%Aladin.Tree        Image/Gamma-ray/Fermi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-11T12:41Z

%ActionName         P-Fermi-Band5.hpx
%Description        Fermi-LAT 3-300 GeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Fermi_Band5
%VerboseDescr       Fermi-LAT all-sky survey in Band 5 (3-300 GeV), at an angular resolution of 0.2 degrees. Units are cnts/s/cm^2/sr. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Fermi/Band5
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Fermi-LAT 3-300 GeV
%Aladin.Tree        Image/Gamma-ray/Fermi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-11T12:43Z

%ActionName         P-Fermi-color.hpx
%Description        Fermi Color HEALPix survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-Fermi-color_0.hpx availability=0
%SeeAction          P-Fermi-color_1.hpx availability=0
%SeeAction          P-Fermi-color_2.hpx availability=0
%VerboseDescr       Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option.
%Copyright          Distributed by SkyView/HEASARC - HEALPixed by CDS
%Origin             CDS
%Id                 P/Fermi/color
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        1
%Aladin.XLabel      Fermi color
%Aladin.Tree        Image/Gamma-ray
%Aladin.MenuNumber  00-01-01 lite
%Aladin.HpxParam    3 image color equatorial jpeg
%Aladin.Date        2016-11-30T14:17Z

%ActionName         P-Finkbeiner.hpx
%Description        Finkbeiner Halpha composite survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-Finkbeiner_0.hpx availability=0
%SeeAction          P-Finkbeiner_1.hpx availability=0
%SeeAction          P-Finkbeiner_2.hpx availability=0
%VerboseDescr       D. Finkbeiner has assembled a full sky Halpha map using data from several surveys: the Wisconsin H-Alpha Mapper (WHAM), the Virginia Tech Spectral-Line Survey (VTSS), and the Southern H-Alpha Sky Survey Atlas (SHASSA). The composite map can be used to provide limits on free-free foreground emission.
%Copyright          Composite map by Douglas Finkbeiner (2004).
%Origin             CDS
%Id                 P/Finkbeiner
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      Finkbeiner Halpha
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.MenuNumber  06-01 lite
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2016-12-01T09:19Z

%ActionName         P-GALEXGR6-AIS-FUV.hpx
%Description        GALEX GR6 AIS (until March 2014)- Far UV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GALEX/GR6-03-2014/AIS-FD
%VerboseDescr       From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position.  Significant updates and improvements have been made to the calibrations used for the GR6 data reductions.
%Copyright          Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract.
%Origin             CDS
%Id                 P/GALEXGR6/AIS/FUV
%Aladin.Profile     >6.1
%Copyright.Url      http://galex.stsci.edu/GR6/
%SkyFraction        0.6821
%Aladin.XLabel      GALEX Allsky Imaging Survey (AIS) FUV
%Aladin.Tree        Image/UV/GALEX
%Aladin.MenuNumber  02-01-03
%Aladin.HpxParam    8 image equatorial png fits
%Aladin.Date        2016-12-02T10:55Z

%ActionName         P-GALEXGR6-AIS-NUV.hpx
%Description        GALEX GR6 AIS (until March 2014)- NEAR UV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GALEX/GR6-03-2014/AIS-ND
%VerboseDescr       From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position.  Significant updates and improvements have been made to the calibrations used for the GR6 data reductions.
%Copyright          Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract.
%Origin             CDS
%Id                 P/GALEXGR6/AIS/NUV
%Aladin.Profile     >6.1
%Copyright.Url      http://galex.stsci.edu/GR6/
%SkyFraction        0.7961
%Aladin.XLabel      GALEX Allsky Imaging Survey (AIS) NUV
%Aladin.Tree        Image/UV/GALEX
%Aladin.MenuNumber  02-01-02
%Aladin.HpxParam    8 image equatorial png fits
%Aladin.Date        2016-12-02T11:00Z

%ActionName         P-GALEXGR6-AIS-color.hpx
%Description        GALEX GR6 AIS (until March 2014)- Color composition
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-GALEXGR6-AIS-color_0.hpx availability=0
%SeeAction          P-GALEXGR6-AIS-color_1.hpx availability=11
%SeeAction          P-GALEXGR6-AIS-color_2.hpx availability=0
%SeeAction          P-GALEXGR6-AIS-color_3.hpx availability=0
%SeeAction          P-GALEXGR6-AIS-color_4.hpx availability=9999
%SeeAction          P-GALEXGR6-AIS-color_5.hpx availability=1055
%SeeAction          P-GALEXGR6-AIS-color_6.hpx availability=14
%VerboseDescr       From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position.  Significant updates and improvements have been made to the calibrations used for the GR6 data reductions.
%Copyright          Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract.
%Origin             CDS
%Id                 P/GALEXGR6/AIS/color
%Aladin.Profile     >6.1
%Copyright.Url      http://galex.stsci.edu/GR6/
%SkyFraction        0.7979
%Aladin.XLabel      GALEX Allsky Imaging Survey (AIS) colored
%Aladin.Tree        Image/UV/GALEX
%Aladin.MenuNumber  02-01-01 lite
%Aladin.HpxParam    8 image color equatorial png jpeg
%Aladin.Date        2016-12-01T14:02Z

%ActionName         P-GALEXGR6_7-color.hpx
%Description        GALEX GR6/7 - Color composition
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1676280807  2023/02/13 11:33:27
%SeeAction          P-GALEXGR6_7-color_0.hpx availability=0
%SeeAction          P-GALEXGR6_7-color_1.hpx availability=0
%SeeAction          P-GALEXGR6_7-color_2.hpx availability=0
%VerboseDescr       The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy. From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). During the course of the mission, the GALEX team have released data to the public through MAST at discrete times. The last complete release was the GR6 (late 2010 through mid 2011 for imaging supplements and the grism survey). A final release of GALEX data arrived in late 2012 at MAST. These included a number of redelivered GR6 data (additional visits and associated coadds from 2003 onwards), along with new tiles within GR7, which span approximately from Jan. 2010 through Feb. 2012
%Copyright          STScI (NASA)
%Origin             CDS
%Id                 P/GALEXGR6_7/color
%Aladin.Profile     >6.1
%Copyright.Url      https://www.stsci.edu/copyright
%SkyFraction        0.7897
%Aladin.XLabel      GALEX
%Aladin.Tree        Image/UV/GALEX
%Aladin.MenuNumber  lite
%Aladin.HpxParam    9 image color equatorial png
%Aladin.Date        2022-03-30T19:35Z

%ActionName         P-GALFAHI-Narrow-DR2.hpx
%Description        GALFAHI Narrow DR2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/GALFAHI/GALFAHI-Narrow-DR2
%VerboseDescr       The Galactic Arecibo L-Band Feed Array H I (GALFA-H I) survey data release 2 (DR2) covers the 21 cm hyperfine transition of Galactic H I from ?650 to 650 {km} {{{s}}}-1, with 0.184 {km} {{{s}}}-1 channel spacing, 4? angular resolution, and 150 mK rms noise per 1 {km} {{{s}}}-1 velocity channel. DR2 covers the entirety of the sky available from the William E. Gordon 305 m antenna at Arecibo, from decl. ?1°17? to decl. + 37°57? across all R.A.: 4 steradians or 32% of the sky. DR2 differs in a number of ways from data release 1, which was released in 2011. DR2 is built from a largely separate set of observations from DR1, which were taken in a much more consistent mode. This consistency, coupled with more careful attention to systematics and more advanced data reduction algorithms, leads to a much higher-quality DR2 data product. We present three data sets for public use: H I data cubes, far-sidelobe stray-radiation-corrected column density maps, and results of the Rolling Hough Transform linear feature detection algorithm.
%Copyright          Regents of the University of Calfornia
%Origin             CDS
%Id                 P/GALFAHI/Narrow/DR2
%Aladin.Profile     >6.1
%Copyright.Url      https://purcell.ssl.berkeley.edu/
%SkyFraction        0.3217
%Aladin.XLabel      GALFAHI Narrow DR2
%Aladin.Tree        Cube
%Aladin.HpxParam    3 cube equatorial png fits
%Aladin.Date        2018-04-12T21:38Z

%ActionName         P-GALFAHI-Wide-DR2.hpx
%Description        GALFAHI Wide DR2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/GALFAHI/GALFAHI-Wide-DR2
%VerboseDescr       The Galactic Arecibo L-Band Feed Array H I (GALFA-H I) survey data release 2 (DR2) covers the 21 cm hyperfine transition of Galactic H I from ?650 to 650 {km} {{{s}}}-1, with 0.184 {km} {{{s}}}-1 channel spacing, 4? angular resolution, and 150 mK rms noise per 1 {km} {{{s}}}-1 velocity channel. DR2 covers the entirety of the sky available from the William E. Gordon 305 m antenna at Arecibo, from decl. ?1°17? to decl. + 37°57? across all R.A.: 4 steradians or 32% of the sky. DR2 differs in a number of ways from data release 1, which was released in 2011. DR2 is built from a largely separate set of observations from DR1, which were taken in a much more consistent mode. This consistency, coupled with more careful attention to systematics and more advanced data reduction algorithms, leads to a much higher-quality DR2 data product. We present three data sets for public use: H I data cubes, far-sidelobe stray-radiation-corrected column density maps, and results of the Rolling Hough Transform linear feature detection algorithm.
%Copyright          Regents of the University of Calfornia
%Origin             CDS
%Id                 P/GALFAHI/Wide/DR2
%Aladin.Profile     >6.1
%Copyright.Url      https://purcell.ssl.berkeley.edu/
%SkyFraction        0.3217
%Aladin.XLabel      GALFAHI Wide DR2
%Aladin.Tree        Cube
%Aladin.HpxParam    3 cube equatorial png fits
%Aladin.Date        2018-04-16T18:04Z

%ActionName         P-GASS+EBHIS.hpx
%Description        HI4PI survey (GASS+EBHIS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/GASS+EBHIS
%VerboseDescr       HI4PI 21-cm survey, an all-sky survey based on the Effelsberg-Bonn HI Survey (EBHIS) and the Parkes Galactic All-Sky Survey (GASS), at an angular resolution of 16.2?. Units: cm-2\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/GASS+EBHIS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      GASS+EBHIS 21-cm
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2018-03-05T09:28Z

%ActionName         P-GASS-NH.hpx
%Description        Parkes Galactic All Sky Survey (GASS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/GASS
%VerboseDescr       21-cm emission from Galactic neutral hydrogen for the entire sky south of delta=+1deg, using the Parkes Radio telescope. The resolution of the map is 16'. Units: H/cm2\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/GASS/NH
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.5241
%Aladin.XLabel      GASS NH
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-07-08T16:10Z

%ActionName         P-GASS.hpx
%Description        Parkes Galactic All Sky Survey (GASS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/GASS.hpx.gz
%VerboseDescr       The Parkes Galactic All Sky Survey (GASS) is a survey of the atomic hydrogen (HI) emission in the Milky Way for the entire sky south of delta = +1deg using the thirteen beam 20 cm multibeam receiver on the Parkes Radio Telescope. GASS covers all Milky Way velocities between LSR -400 km/s and 500 km/s. GASS is the most sensitive fully-sampled survey of Galactic HI ever made in the Southern sky. Survey goals include a better understanding of the interaction of the Milky Way disk and halo and the nature of high and intermediate velocity clouds (HVCs and IVCs).\n\nSee the reference article: McClure-Griffiths et al. ApJS 181, 2009
%Copyright          from CSIRO/ATNF - healpixed by CDS
%Id                 P/GASS
%Origin             CDS
%Copyright.url      http://www.atnf.csiro.au/research/GASS/index.html
%Aladin.Profile     >6.1
%Aladin.XLabel      GASS
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.HpxParam    map
%Aladin.MenuNumber  06-06

%ActionName         P-GAURIBIDANUR.hpx
%Description        Gauribidanur 35 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/GAURIBIDANUR
%VerboseDescr       Northern sky survey at 34.5 MHz using the low frequency telescope at Gauribidanur. The synthesized beam has a resolution of 26?x42?sec(delta-14.1deg) Units:KTB \nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/GAURIBIDANUR
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.8623
%Aladin.XLabel      GAURIBIDANUR
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-09-01T14:27Z

%ActionName         P-GLIMPSE360.hpx
%Description        GLIMPSE360: Spitzer's Infrared Milky Way
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1461233435  2016/04/21 12:10:35
%Url                http://www.spitzer.caltech.edu/glimpse360/aladin/data
%VerboseDescr       This infrared view of the disk, or plane, of our Milky Way galaxy is assembled from more than 2 million snapshots taken over the past 10 years by NASA's Spitzer Space Telescope. The data were taken as part of a huge survey project called the Galactic Legacy Mid-Plane Survey Extraordinaire, or GLIMPSE360. Spitzer spent a total of 172 days taking the individual pictures, and this is the first time they have been stitched together into a single expansive view. The image covers about 3% of our sky, but because it focuses on a band of the sky that includes the plane of our galaxy, it shows more than half of the Milky Way's stars. The blue dots throughout the image are all individual stars, most of which are relatively close to us, while the blue haze towards the galactic center is also made up of starlight, too far away for us to pick out individual stars, but all contributing to the glow. The red structures are clouds of dust and gas that permeate our galaxy, and give birth to new stars. Throughout the image, you can see star birth in action, in brightly-lit regions; look closely and you'll also see bubbles, pillars and other shapes blown out and carved in the dust and gas by starlight and stellar winds. In many areas, dark filaments stand out sharply against the bright background. These dark tendrils are the thickest dust clouds in our galaxy, that not even Spitzer's infrared view can penetrate. The image combines data from multiple surveys: GLIMPSE, GLIMPSEII, GLIMPSE3D, Vela-Carina, GLIMPSE360, Deep GLIMPSE, CYGX, GALCEN, & SMOG. The 12-micron data from NASA's Wide-field Infrared Survey Explorer (WISE) was substituted for missing 8-micron data in outer galaxy regions mapped during Spitzer's post-cryo mission.
%Copyright          Spitzer mission - JPL/NASA
%Origin             IPAC
%Id                 P/GLIMPSE360
%Aladin.Profile     >6.1
%SkyFraction        0.03121
%Aladin.XLabel      GLIMPSE360
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-0 lite
%Aladin.HpxParam    9 image color equatorial jpeg
%Aladin.Date        2013-11-29T17:38Z

%ActionName         P-Ganymede-VoyagerGalileo-SSI-1km.hpx
%Description        Ganymede VoyagerGalileo SSI 1km
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Ganymede_VoyagerGalileo-SSI-1km
%VerboseDescr       This global mosaic of Ganymede utilizes the best image quality and moderate resolution coverage supplied by Galileo Solid-State Imaging (SSI) and Voyager 1 and 2. This mosaic was prepared by the USGS Astrogeology Science Center using the ISIS 2 image processing and cartographic system. The image data was selected on the basis of overall image quality, reasonable input resolution (from 20 km/pixel for gap fill to approximately 400 meters/pixel), and availability of moderate viewing and sun angles for topography.
%Copyright          USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Ganymede/VoyagerGalileo-SSI-1km
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Ganymede/VoyagerGalileo-SSI-1km
%Aladin.Tree        Solar system/Jupiter/Ganymede
%Aladin.HpxParam    3 image color ganymede jpeg
%Aladin.Date        2018-01-16T15:12Z

%ActionName         P-HERSCHEL-PACS-color.hpx
%Description        Herschel PACS (color composition)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Herschel/PACS-color
%VerboseDescr       A color composition using all public PACS observations from the Herschel Science Archive at 70 micron (blue) and 160 micron (red).
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS-color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.0835
%Aladin.XLabel      PACS-color
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image color equatorial jpeg
%Aladin.Date        2015-10-16T01:02Z

%ActionName         P-HERSCHEL-PACS100.hpx
%Description        Herschel PACS 100 micron
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Herschel/PACS100
%VerboseDescr       All public PACS-100 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS100
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.03605
%Aladin.XLabel      PACS-100micron
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image equatorial jpeg png fits
%Aladin.Date        2015-09-02T16:39Z

%ActionName         P-HERSCHEL-PACS100norm.hpx
%Description        PACS100 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/PACS_hips100/
%VerboseDescr       All public level-2.5 PACS-100 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS100norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.02426
%Aladin.XLabel      PACS100 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image equatorial png fits
%Aladin.Date        2017-09-27T11:39Z

%ActionName         P-HERSCHEL-PACS160.hpx
%Description        Herschel PACS 160 micron
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Herschel/PACS160
%VerboseDescr       All public PACS-160 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS160
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.08346
%Aladin.XLabel      PACS-160micron
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    8 image equatorial jpeg png fits
%Aladin.Date        2015-09-02T16:23Z

%ActionName         P-HERSCHEL-PACS160norm.hpx
%Description        PACS160 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/PACS_hips160/
%VerboseDescr       All public level-2.5 PACS-160 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS160norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.06995
%Aladin.XLabel      PACS160 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    8 image equatorial png fits
%Aladin.Date        2017-09-26T17:14Z

%ActionName         P-HERSCHEL-PACS70.hpx
%Description        Herschel PACS 70 micron
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Herschel/PACS70
%VerboseDescr       All public PACS-70 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS70
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.04222
%Aladin.XLabel      PACS-70micron
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image equatorial jpeg png fits
%Aladin.Date        2015-09-02T16:55Z

%ActionName         P-HERSCHEL-PACS70norm.hpx
%Description        PACS70 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/PACS_hips70/
%VerboseDescr       All public level-2.5 PACS-70 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS70norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.05145
%Aladin.XLabel      PACS70 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image equatorial png fits
%Aladin.Date        2017-09-27T17:55Z

%ActionName         P-HERSCHEL-PACS_RGB_norm.hpx
%Description        PACS RGB 70+160 micron norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/PACS_hipsRGB/
%VerboseDescr       A color composition using all public PACS observations from the Herschel Science Archive at 70 micron (blue) and 160 micron (red), with the green colour being the average between the two bands. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/PACS_RGB_norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.05599
%Aladin.XLabel      PACS RGB 70+160 micron norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    9 image color equatorial png
%Aladin.Date        2017-09-26T13:23Z

%ActionName         P-HERSCHEL-SPIRE-250.hpx
%Description        SPIRE250
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/SPIRE250
%VerboseDescr       All public SPIRE-250 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE-250
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.1545
%Aladin.XLabel      SPIRE250
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    7 image live equatorial png fits
%Aladin.Date        2016-07-13T15:54Z

%ActionName         P-HERSCHEL-SPIRE-350.hpx
%Description        SPIRE350
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/SPIRE350
%VerboseDescr       All public SPIRE-350 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE-350
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.2492
%Aladin.XLabel      SPIRE350
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    6 image live equatorial png fits
%Aladin.Date        2016-07-13T12:08Z

%ActionName         P-HERSCHEL-SPIRE-500.hpx
%Description        Herschel SPIRE 500 micron
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/SPIRE500
%VerboseDescr       All public SPIRE-500 observations from the Herschel Science Archive.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE-500
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.458
%Aladin.XLabel      SPIRE500
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    5 image live equatorial png fits
%Aladin.Date        2016-07-13T11:16Z

%ActionName         P-HERSCHEL-SPIRE-RGBnorm.hpx
%Description        -- missing description --
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/normalized/SPIRE_pnorm_RGB/
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE/RGBnorm
%Aladin.Profile     >6.1
%Aladin.XLabel      P/HERSCHEL/SPIRE/RGBnorm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    
%Aladin.Date        2017-08-19T10:30Z

%ActionName         P-HERSCHEL-SPIRE-color.hpx
%Description        Herschel SPIRE (color composition)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/SPIRE-color
%VerboseDescr       A color composition using all public SPIRE observations from the Herschel Science Archive at 250 micron (blue), 350 micron (green) and 500 micron (red).
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE-color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.4582
%Aladin.XLabel      SPIRE-color
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    7 image color live equatorial png jpeg
%Aladin.Date        2016-07-14T16:13Z

%ActionName         P-HERSCHEL-SPIRE250norm.hpx
%Description        SPIRE250 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/hips250_pnorm_allsky/
%VerboseDescr       All public SPIRE-250 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE250norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.08737
%Aladin.XLabel      SPIRE250 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2017-08-18T19:46Z

%ActionName         P-HERSCHEL-SPIRE350norm.hpx
%Description        SPIRE350 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/hips350_pnorm_allsky/
%VerboseDescr       All public SPIRE-350 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE350norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.08985
%Aladin.XLabel      SPIRE350 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    6 image equatorial png fits
%Aladin.Date        2017-08-18T18:46Z

%ActionName         P-HERSCHEL-SPIRE500norm.hpx
%Description        SPIRE500 norm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://skies.esac.esa.int/Herschel/normalized/hips500_pnorm_allsky/
%VerboseDescr       All public SPIRE-350 observations from the Herschel Science Archive. The data have been normalised using Herschel-optimised cuts and stretch prior to the HiPS generation.
%Copyright          ESA/HSA
%Origin             ESAVO
%Id                 P/HERSCHEL/SPIRE500norm
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/herschel/publishing-rules-guidelines
%SkyFraction        0.09361
%Aladin.XLabel      SPIRE500 norm
%Aladin.Tree        Image/Infrared/HERSCHEL
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2017-08-18T18:30Z

%ActionName         P-HGPS-Flux.hpx
%Description        HGPS integral flux > 1 TeV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/pub/10.1051_0004-6361_201732098flux
%VerboseDescr       H.E.S.S. is an array of ground-based gamma-ray telescopes located in Namibia. The H.E.S.S. Galactic Plane Survey (HGPS) is the first deep and wide survey of the Milky Way in TeV gamma-rays. The flux values are given as integral photon flux above 1 TeV assuming a power law spectrum for the differential flux with an index of -2.3. The pixel values represent integrated values within a circular region of 0.1 deg.
%Origin             CDS
%Id                 P/HGPS/Flux
%Aladin.Profile     >6.1
%SkyFraction        0.03253
%Aladin.XLabel      HGPS
%Aladin.Tree        Image/Gamma-ray/HESS
%Aladin.HpxParam    3 image color equatorial png
%Aladin.Date        2018-07-07T13:47Z

%ActionName         P-HGPS-Significance.hpx
%Description        HGPS significance (Gaussian sigma)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/pub/10.1051_0004-6361_201732098significance
%VerboseDescr       H.E.S.S. is an array of ground-based gamma-ray telescopes located in Namibia. The H.E.S.S. Galactic Plane Survey (HGPS) is the first deep and wide survey of the Milky Way in TeV gamma-rays. The flux values are given as integral photon flux above 1 TeV assuming a power law spectrum for the differential flux with an index of -2.3. The pixel values represent integrated values within a circular region of 0.1 deg.
%Origin             CDS
%Id                 P/HGPS/Significance
%Aladin.Profile     >6.1
%SkyFraction        0.03253
%Aladin.XLabel      HGPS
%Aladin.Tree        Image/Gamma-ray/HESS
%Aladin.HpxParam    3 image color equatorial png
%Aladin.Date        2018-07-07T13:47Z

%ActionName         P-HI.hpx
%Description        HI composite survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/HI
%VerboseDescr       Composite all-sky map of neutral hydrogen column density (N_HI), formed from the Leiden/Dwingeloo HI survey data (Hartmann & Burton 1997) and the composite N_HI map of Dickey and Lockman (1990). The two datasets are not matched in sensitivity or resolution: note that discontinuities exist in the constructed composite map. A pixel mask is provided to indicate which dataset was used for each location on the sky. Hartmann & Burton provide a velocity integrated (-450 km/s < V_lsr < +400 km/s) HI brightness temperature map in Galactic coordinates, sampled every 0.5 degrees. This entire data set was converted to N_HI by multiplying by their factor of 1.8224e18 K km s-1 cm-2 and then interpolated to pixel centers appropriate for HEALPix Nside=512. Since the Leiden/Dwingeloo survey does not have sky coverage for declinations < -30 deg., the lower resolution Dickey & Lockman map was also interpolated to HEALPix and used to fill in the coverage gap. The Dickey & Lockman N_HI map is itself a composite of several surveys which had been merged and averaged onto 1 deg. bins in Galactic coordinates. Their map includes emission between -250 km/s < V_lsr < 250 km/s (excluding the LMC and SMC). The Leiden/Dwingeloo Survey data were obtained from the CDS. The Dickey & Lockman map was obtained from NCSA ADIL. This original HEALPix file is distributed and maintained by LAMBDA.
%Copyright          Composite HI map by LAMBDA
%Origin             CDS
%Id                 P/HI
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/foreground/fg_HI_get.cfm
%SkyFraction        1
%Aladin.XLabel      HI
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.MenuNumber  06-05
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2014-04-19T17:59Z

%ActionName         P-HI4PI-NHI.hpx
%Description        HI4PI NHI survey (full-sky HI column density distribution)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HI4PI/P_HI4PI_NHI
%VerboseDescr       The HI4PI data release comprises 21-cm neutral atomic hydrogen data of the Milky Way (-600km/s<vlsr<+600km/s for declination >0deg; -470km/s<vlsr<+470km/s for declination <0deg) as observed with the 100-m radio telescope at Effelsberg and the 64-m radio telescope at Parkes. HI4PI covers the full 4-pi sky.
%Copyright          VizieR Service, CDS (ftp : J/A+A/594/A116/)
%Origin             CDS
%Id                 P/HI4PI/NHI
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      HI4PI NHI
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2017-06-12T13:36Z

%ActionName         P-HITOMI-HXI.hpx
%Description        Hitomi HXI public data image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/hitomi_hxi
%VerboseDescr       Superposition of Hitomi pseudo-color images, no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/HITOMI-HXI
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/hitomi
%SkyFraction        1
%Aladin.XLabel      Hitomi
%Aladin.Tree        Image/X
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2017/04/18 16:02:32

%ActionName         P-HITOMI-SXI.hpx
%Description        Hitomi SXI public data image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/hitomi_sxi
%VerboseDescr       Superposition of Hitomi pseudo-color images, no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/HITOMI-SXI
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/hitomi
%SkyFraction        1
%Aladin.XLabel      Hitomi
%Aladin.Tree        Image/X
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2017/04/18 16:02:32

%ActionName         P-HITOMI-SXS.hpx
%Description        Hitomi SXS public data image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/hitomi_sxs
%VerboseDescr       Superposition of Hitomi pseudo-color images, no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/HITOMI-SXS
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/hitomi
%SkyFraction        1
%Aladin.XLabel      Hitomi
%Aladin.Tree        Image/X
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2017/04/18 16:02:32

%ActionName         P-HLA-B.hpx
%Description        HLA-B : F450W, F439W, F438W, F435W and F430W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_B_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets to
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/B
%Aladin.Profile     >6.1
%SkyFraction        2.254E-4
%Aladin.XLabel      HLA-B
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T11:14Z

%ActionName         P-HLA-CO.hpx
%Description        HLA-CO : F222M
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_CO_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/CO
%Aladin.Profile     >6.1
%SkyFraction        3.404E-6
%Aladin.XLabel      HLA-CO
%Aladin.Tree        Image/Gas-lines/CO
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-10T17:54Z

%ActionName         P-HLA-H.hpx
%Description        HLA-H : F160W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_H_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/H
%Aladin.Profile     >6.1
%SkyFraction        1.912E-4
%Aladin.XLabel      HLA-H
%Aladin.Tree        Image/Infrared/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T17:21Z

%ActionName         P-HLA-H2O.hpx
%Description        HLA-H2O : F139M
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_H2O_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/H2O
%Aladin.Profile     >6.1
%SkyFraction        1.598E-5
%Aladin.XLabel      HLA-H2O
%Aladin.Tree        Image/Gas-lines/H2O
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-10T18:22Z

%ActionName         P-HLA-Halpha.hpx
%Description        HLA-Halpha : F656N and F657N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_Halpha_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/Halpha
%Aladin.Profile     >6.1
%SkyFraction        5.049E-5
%Aladin.XLabel      HLA-Halpha
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-10T19:07Z

%ActionName         P-HLA-Hbeta.hpx
%Description        HLA-Hbeta : F487N and F486N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_Hbeta_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/Hbeta
%Aladin.Profile     >6.1
%SkyFraction        3.880E-6
%Aladin.XLabel      HLA-Hbeta
%Aladin.Tree        Image/Gas-lines/Hbeta
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T05:22Z

%ActionName         P-HLA-I.hpx
%Description        HLA-I : F814W, F791W, F785LP and F775W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_I_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/I
%Aladin.Profile     >6.1
%SkyFraction        8.996E-4
%Aladin.XLabel      HLA-I
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-17T09:32Z

%ActionName         P-HLA-J.hpx
%Description        HLA-J : F140W, F125W, F125LP and F115LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_J_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/J
%Aladin.Profile     >6.1
%SkyFraction        6.400E-5
%Aladin.XLabel      HLA-J
%Aladin.Tree        Image/Infrared/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T13:55Z

%ActionName         P-HLA-NII.hpx
%Description        HLA-NII : F658N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_NII_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/NII
%Aladin.Profile     >6.1
%SkyFraction        6.177E-5
%Aladin.XLabel      HLA-NII
%Aladin.Tree        Image/Gas-lines/NII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T22:45Z

%ActionName         P-HLA-OII.hpx
%Description        HLA-OII : F375N and F373N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_OII_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/OII
%Aladin.Profile     >6.1
%SkyFraction        3.967E-6
%Aladin.XLabel      HLA-OII
%Aladin.Tree        Image/Gas-lines/OII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-12T06:58Z

%ActionName         P-HLA-OIII.hpx
%Description        HLA-OIII : F502N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_OIII_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/OIII
%Aladin.Profile     >6.1
%SkyFraction        3.848E-5
%Aladin.XLabel      HLA-OIII
%Aladin.Tree        Image/Gas-lines/OIII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-12T07:51Z

%ActionName         P-HLA-Palpha.hpx
%Description        HLA-Palpha : F187N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_Palpha_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/Palpha
%Aladin.Profile     >6.1
%SkyFraction        4.111E-6
%Aladin.XLabel      HLA-Palpha
%Aladin.Tree        Image/Gas-lines/Palpha
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T05:31Z

%ActionName         P-HLA-Palpha_c.hpx
%Description        HLA-Palpha_c : F190W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_Palpha_c_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/Palpha_c
%Aladin.Profile     >6.1
%SkyFraction        4.132E-6
%Aladin.XLabel      HLA-Palpha_c
%Aladin.Tree        Image/Gas-lines/Palphac
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-11T05:28Z

%ActionName         P-HLA-R.hpx
%Description        HLA-R : F702W and F675W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_R_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/R
%Aladin.Profile     >6.1
%SkyFraction        8.210E-5
%Aladin.XLabel      HLA-R
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-14T06:48Z

%ActionName         P-HLA-SDSSg.hpx
%Description        HLA-SDSSg : F475W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_SDSSg_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/SDSSg
%Aladin.Profile     >6.1
%SkyFraction        1.167E-4
%Aladin.XLabel      HLA-SDSSg
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-10T17:25Z

%ActionName         P-HLA-SDSSr.hpx
%Description        HLA-SDSSr : F625W and F622W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_SDSSr_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/SDSSr
%Aladin.Profile     >6.1
%SkyFraction        4.937E-5
%Aladin.XLabel      HLA-SDSSr
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-10T11:44Z

%ActionName         P-HLA-SDSSz.hpx
%Description        HLA-SDSSz : F850LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_SDSSz_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/SDSSz
%Aladin.Profile     >6.1
%SkyFraction        1.097E-4
%Aladin.XLabel      HLA-SDSSz
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-12T14:26Z

%ActionName         P-HLA-SIII.hpx
%Description        HLA-SIII : F873N, FQ672N and FQ674N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_SIII_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/SIII
%Aladin.Profile     >6.1
%SkyFraction        3.381E-5
%Aladin.XLabel      HLA-SIII
%Aladin.Tree        Image/Gas-lines/SIII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-12T11:51Z

%ActionName         P-HLA-U.hpx
%Description        HLA-U : F336W, F330W, F300W, F275W and F342W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_U_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/U
%Aladin.Profile     >6.1
%SkyFraction        2.376E-4
%Aladin.XLabel      HLA-U
%Aladin.Tree        Image/UV/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-12T21:14Z

%ActionName         P-HLA-UV.hpx
%Description        HLA-UV : F170W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_UV_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/UV
%Aladin.Profile     >6.1
%SkyFraction        9.788E-6
%Aladin.XLabel      HLA-UV
%Aladin.Tree        Image/UV/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-13T09:43Z

%ActionName         P-HLA-V.hpx
%Description        HLA-V : F555W, F547W, F569W and F550W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_V_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/V
%Aladin.Profile     >6.1
%SkyFraction        2.223E-4
%Aladin.XLabel      HLA-V
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-13T13:51Z

%ActionName         P-HLA-Y.hpx
%Description        HLA-Y : F110W and F105W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_Y_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets to
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/Y
%Aladin.Profile     >6.1
%SkyFraction        1.146E-4
%Aladin.XLabel      HLA-Y
%Aladin.Tree        Image/Infrared/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-14T08:46Z

%ActionName         P-HLA-wideUV.hpx
%Description        HLA-wideUV : F255W, F250W, F225W, F220W and F218W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_wideUV_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets tog
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/wideUV
%Aladin.Profile     >6.1
%SkyFraction        5.728E-5
%Aladin.XLabel      HLA-wideUV
%Aladin.Tree        Image/UV/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-15T10:00Z

%ActionName         P-HLA-wideV.hpx
%Description        HLA-wideV : F606W and F600LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/HLA-hips/filter_wideV_hips
%VerboseDescr       The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets to
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HLA/wideV
%Aladin.Profile     >6.1
%SkyFraction        6.482E-4
%Aladin.XLabel      HLA-wideV
%Aladin.Tree        Image/Optical/HST/HLA
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-04-15T07:50Z

%ActionName         P-HST-B.hpx
%Description        HST-B includes the following filters: F450W, F439W, F438W, F435W and F430W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_B_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F450W, F439W, F438W, F435W and F430W filters between the beginning of the mission to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/B
%Aladin.Profile     >6.1
%SkyFraction        1.590E-4
%Aladin.XLabel      HST-B
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-25T21:55Z

%ActionName         P-HST-CO.hpx
%Description        HST-CO includes the following filters: F222M
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_CO_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F222W filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/CO
%Aladin.Profile     >6.1
%SkyFraction        4.351E-6
%Aladin.XLabel      HST-CO
%Aladin.Tree        Image/Gas-lines/CO
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-21T19:09Z

%ActionName         P-HST-GOODS-b.hpx
%Description        GOODS b
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GOODS/GOODSb
%VerboseDescr       The P/HST/GOODS/b Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F435W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Origin             CDS
%Id                 P/HST/GOODS/b
%Aladin.Profile     >6.1
%Copyright.Url      http://www.stsci.edu/institute/Copyright
%SkyFraction        2.223E-6
%Aladin.XLabel      HST GOODS b
%Aladin.Tree        Image/Optical/HST/GOODS
%Aladin.MenuNumber  03-05-02-01
%Aladin.HpxParam    14 image equatorial png fits
%Aladin.Date        2017-03-27T14:34Z

%ActionName         P-HST-GOODS-color.hpx
%Description        GOODS color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GOODS/GOODS-color
%VerboseDescr       The P/HST/GOODS/color Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in v,i and z bands as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities,\nto survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Origin             CDS
%Id                 P/HST/GOODS/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.stsci.edu/institute/Copyright
%SkyFraction        2.650E-6
%Aladin.XLabel      HST GOODS color
%Aladin.Tree        Image/Optical/HST/GOODS
%Aladin.MenuNumber  03-05-02-00
%Aladin.HpxParam    14 image color equatorial png
%Aladin.Date        2017-03-27T15:14Z

%ActionName         P-HST-GOODS-i.hpx
%Description        GOODS i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GOODS/GOODSi
%VerboseDescr       The P/HST/GOODS/i Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F435W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities,\nto survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Origin             CDS
%Id                 P/HST/GOODS/i
%Aladin.Profile     >6.1
%Copyright.Url      http://www.stsci.edu/institute/Copyright
%SkyFraction        2.628E-6
%Aladin.XLabel      HST GOODS i
%Aladin.Tree        Image/Optical/HST/GOODS
%Aladin.MenuNumber  03-05-02-03
%Aladin.HpxParam    14 image equatorial png fits
%Aladin.Date        2017-03-27T15:03Z

%ActionName         P-HST-GOODS-v.hpx
%Description        GOODS v
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GOODS/GOODSv
%VerboseDescr       The P/HST/GOODS/v Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F435W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Origin             CDS
%Id                 P/HST/GOODS/v
%Aladin.Profile     >6.1
%Copyright.Url      http://www.stsci.edu/institute/Copyright
%SkyFraction        2.626E-6
%Aladin.XLabel      HST GOODS v
%Aladin.Tree        Image/Optical/HST/GOODS
%Aladin.MenuNumber  03-05-02-02
%Aladin.HpxParam    14 image equatorial png fits
%Aladin.Date        2017-03-27T15:07Z

%ActionName         P-HST-GOODS-z.hpx
%Description        GOODS z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/GOODS/GOODSz
%VerboseDescr       The P/HST/GOODS/z Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F435W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum.
%Copyright          NASA/ESA/AURA
%Origin             CDS
%Id                 P/HST/GOODS/z
%Aladin.Profile     >6.1
%Copyright.Url      http://www.stsci.edu/institute/Copyright
%SkyFraction        2.512E-6
%Aladin.XLabel      HST GOODS z
%Aladin.Tree        Image/Optical/HST/GOODS
%Aladin.MenuNumber  03-05-02-04
%Aladin.HpxParam    14 image equatorial png fits
%Aladin.Date        2017-03-27T15:10Z

%ActionName         P-HST-H.hpx
%Description        HST-H includes the following filters: F160W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_H_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F160W filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/H
%Aladin.Profile     >6.1
%SkyFraction        1.595E-4
%Aladin.XLabel      HST-H
%Aladin.Tree        Image/Infrared/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-25T23:43Z

%ActionName         P-HST-H2O.hpx
%Description        HST-H2O includes the following filters: F139M
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_H2O_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F139M filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/H2O
%Aladin.Profile     >6.1
%SkyFraction        2.049E-5
%Aladin.XLabel      HST-H2O
%Aladin.Tree        Image/Gas-lines/H2O
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-05T20:01Z

%ActionName         P-HST-Halpha.hpx
%Description        HST-Halpha includes the following filters: F656N and F657N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_Halpha_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F656N and F657N filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/Halpha
%Aladin.Profile     >6.1
%SkyFraction        3.518E-5
%Aladin.XLabel      HST-Halpha
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-06T02:06Z

%ActionName         P-HST-Hbeta.hpx
%Description        HST-Hbeta includes the following filters: F487N and F486N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_Hbeta_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F487N and F486N filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/Hbeta
%Aladin.Profile     >6.1
%SkyFraction        2.906E-6
%Aladin.XLabel      HST-Hbeta
%Aladin.Tree        Image/Gas-lines/Hbeta
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-05T20:07Z

%ActionName         P-HST-I.hpx
%Description        HST-I includes the following filters: F814W, F791W, F785LP and F775W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_I_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F814W, F791W, F785LP and F775W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/I
%Aladin.Profile     >6.1
%SkyFraction        7.058E-4
%Aladin.XLabel      HST-I
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-03-01T03:14Z

%ActionName         P-HST-J.hpx
%Description        HST-J includes the following filters: F140W, F125W, F125LP and F115LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_J_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F140W, F125W, F125LP and F115LP filters between the beginning of the mission to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/J
%Aladin.Profile     >6.1
%SkyFraction        5.139E-5
%Aladin.XLabel      HST-J
%Aladin.Tree        Image/Infrared/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-23T20:20Z

%ActionName         P-HST-NII.hpx
%Description        HST-NII includes the following filters: F658N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_NII_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F658N filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/NII
%Aladin.Profile     >6.1
%SkyFraction        4.909E-5
%Aladin.XLabel      HST-NII
%Aladin.Tree        Image/Gas-lines/NII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-06T16:21Z

%ActionName         P-HST-OII.hpx
%Description        HST-OII includes the following filters: F375N and F373N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_OII_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F375N and F373N filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Origin             CDS
%Id                 P/HST/OII
%Aladin.Profile     >6.1
%SkyFraction        2.521E-6
%Aladin.XLabel      HST-OII
%Aladin.Tree        Image/Gas-lines/OII
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-27T15:38Z

%ActionName         P-HST-OIII.hpx
%Description        HST-OIII includes the following filters: F502N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_OIII_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F502N filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/OIII
%Aladin.Profile     >6.1
%SkyFraction        2.558E-5
%Aladin.XLabel      HST-OIII
%Aladin.Tree        Image/Gas-lines/OIII
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-21T20:09Z

%ActionName         P-HST-PHAT-F110W.hpx
%Description        HST PHAT - F110W - WFC3/IR
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F110W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F110W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.204E-5
%Aladin.XLabel      HST PHAT F110W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-01
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-03T11:17Z

%ActionName         P-HST-PHAT-F160W.hpx
%Description        HST PHAT - F160W - WFC3/IR
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F160W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F160W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.205E-5
%Aladin.XLabel      HST PHAT F160W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-02
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-03T16:13Z

%ActionName         P-HST-PHAT-F275W.hpx
%Description        HST PHAT - F275W - WFC3/UVIS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F275W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F275W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.263E-5
%Aladin.XLabel      HST PHAT F275W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-02
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-04T13:43Z

%ActionName         P-HST-PHAT-F336W.hpx
%Description        HST PHAT - F336W - WFC3/UVIS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F336W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F336W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.263E-5
%Aladin.XLabel      HST PHAT F336W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-04
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-05T17:14Z

%ActionName         P-HST-PHAT-F475W.hpx
%Description        HST PHAT - F475W - ACS/WFC
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F475W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F475W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.338E-5
%Aladin.XLabel      HST PHAT F475W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-05
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-06T12:36Z

%ActionName         P-HST-PHAT-F814W.hpx
%Description        HST PHAT - F814W - ACS/WFC
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/PHAT/F814W
%VerboseDescr       The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D
%Copyright          PHAT team
%Origin             CDS
%Id                 P/HST/PHAT/F814W
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astro.washington.edu/groups/phat/Home.html
%SkyFraction        1.339E-5
%Aladin.XLabel      HST PHAT F814W
%Aladin.Tree        Image/Optical/HST/PHAT
%Aladin.MenuNumber  03-05-05-06
%Aladin.HpxParam    14 image equatorial png jpeg fits
%Aladin.Date        2015-02-10T02:50Z

%ActionName         P-HST-Palpha.hpx
%Description        HST-Palpha includes the following filters: F187N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_Palpha_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F187N filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/Palpha
%Aladin.Profile     >6.1
%SkyFraction        6.035E-6
%Aladin.XLabel      HST-Palpha
%Aladin.Tree        Image/Gas-lines/Palpha
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-05T20:14Z

%ActionName         P-HST-Palpha_c.hpx
%Description        HST-Palpha_c includes the following filters: F190W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_Palpha_c_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F190W filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/Palpha_c
%Aladin.Profile     >6.1
%SkyFraction        4.719E-6
%Aladin.XLabel      HST-Palpha_c
%Aladin.Tree        Image/Gas-lines/Palphac
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-22T16:43Z

%ActionName         P-HST-R.hpx
%Description        HST-R includes the following filters: F702W and F675W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_R_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F702W and F675W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/R
%Aladin.Profile     >6.1
%SkyFraction        4.811E-5
%Aladin.XLabel      HST-R
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-06T00:18Z

%ActionName         P-HST-SDSSg.hpx
%Description        HST-SDSSg incudes the following filters: F475W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_SDSSg_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F475W filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/SDSSg
%Aladin.Profile     >6.1
%SkyFraction        9.929E-5
%Aladin.XLabel      HST-SDSSg
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-23T18:31Z

%ActionName         P-HST-SDSSr.hpx
%Description        HST-SDSSr includes the following filters: F625W and F622W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_SDSSr_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F625W and F622W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/SDSSr
%Aladin.Profile     >6.1
%SkyFraction        4.001E-5
%Aladin.XLabel      HST-SDSSr
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-21T23:34Z

%ActionName         P-HST-SDSSz.hpx
%Description        HST-SDSSz includes the following filters: F850LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_SDSSz_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F850LP filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/SDSSz
%Aladin.Profile     >6.1
%SkyFraction        8.478E-5
%Aladin.XLabel      HST-SDSSz
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-28T21:49Z

%ActionName         P-HST-SIII.hpx
%Description        HST-SIII includes the following filters: F873N, FQ672N and FQ674N
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_SIII_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F873N, FQ672N and FQ674N filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/SIII
%Aladin.Profile     >6.1
%SkyFraction        1.771E-5
%Aladin.XLabel      HST-SIII
%Aladin.Tree        Image/Gas-lines/SIII
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-22T00:10Z

%ActionName         P-HST-U.hpx
%Description        HST-U includes the following filters: F336W, F330W, F300W, F275W and F342W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_U_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F336W, F330W, F300W, F275W and F342W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/U
%Aladin.Profile     >6.1
%SkyFraction        1.666E-4
%Aladin.XLabel      HST-U
%Aladin.Tree        Image/UV/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-03-01T06:18Z

%ActionName         P-HST-UV.hpx
%Description        HST-UV includes the following filters: F170W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_UV_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F170W filter between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/UV
%Aladin.Profile     >6.1
%SkyFraction        7.455E-6
%Aladin.XLabel      HST-UV
%Aladin.Tree        Image/UV/HST
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-05T20:38Z

%ActionName         P-HST-V.hpx
%Description        HST-V includes the following filters: F555W, F547W, F569W and F550W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_V_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F555W, F547W, F569W and F550W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/V
%Aladin.Profile     >6.1
%SkyFraction        1.449E-4
%Aladin.XLabel      HST-V
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-22T23:45Z

%ActionName         P-HST-Y.hpx
%Description        HST-Y includes the following filters: F110W and F105W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_Y_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F110W and F105W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/Y
%Aladin.Profile     >6.1
%SkyFraction        9.598E-5
%Aladin.XLabel      HST-Y
%Aladin.Tree        Image/Infrared/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-23T03:40Z

%ActionName         P-HST-other.hpx
%Description        HST-Others includes the ALL the other filters not used in other HIPS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_other_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done with filters NOT included within the other HIPS between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/other
%Aladin.Profile     >6.1
%SkyFraction        1.027E-4
%Aladin.XLabel      HST-Others
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-02-22T02:51Z

%ActionName         P-HST-wideUV.hpx
%Description        HST-wideUV includes the following filters: F255W, F250W, F225W, F220W and F218W
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_wideUV_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F255W, F250W, F225W, F220W and F218W filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/wideUV
%Aladin.Profile     >6.1
%SkyFraction        3.906E-5
%Aladin.XLabel      HST-wideUV
%Aladin.Tree        Image/UV/HST
%Aladin.HpxParam    13 image live equatorial png fits
%Aladin.Date        2018-11-06T23:15Z

%ActionName         P-HST-wideV.hpx
%Description        HST-wideV includes the following filters: F606W and F600LP
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/HST-hips/filter_wideV_hips
%VerboseDescr       The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F606W and F600LP filters between the beginning of the mission  to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis.
%Copyright          Canadian Astronomy Data Centre
%Origin             CDS
%Id                 P/HST/wideV
%Aladin.Profile     >6.1
%SkyFraction        4.922E-4
%Aladin.XLabel      HST-wideV
%Aladin.Tree        Image/Optical/HST
%Aladin.HpxParam    13 image equatorial png fits
%Aladin.Date        2019-03-03T05:33Z

%ActionName         P-Haslam408-v2.hpx
%Description        Haslam 408Mhz reprocessed
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/Haslam408_2014
%VerboseDescr       Remazeilles et al. 2014 have re-evaluated and re-processed the rawest Haslam 408 MHz data, available from the Max Planck Institute for Radioastronomy Survey Sampler website, to produce an improved source-subtracted and destriped 408 MHz all-sky map. Large-scale striations associated with correlated low-frequency noise in the scan direction are reduced using a Fourier-based filtering technique. The most important improvement results from the removal of extra-galactic sources. An iterative combination of two techniques - two-dimensional Gaussian fitting and minimum curvature spline surface inpainting - are used to remove the brightest sources (with flux density larger than 2 Jy).Desources destrier map.
%Copyright          LAMBDA/NASA
%Origin             CDS
%Id                 P/Haslam408/v2
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/foreground/2014_haslam_408_info.cfm
%SkyFraction        1
%Aladin.XLabel      Haslam 408Mhz reprocessed
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-08a
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-12-20T14:53Z

%ActionName         P-Haslam408.hpx
%Description        Haslam 408MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/Haslam408
%VerboseDescr       The survey data were obtained from the archives of the NCSA ADIL in equatorial 1950 coordinates, and subsequently processed further in the Fourier domain to mitigate baseline striping and strong point sources.  The data were then interpolated onto a Galactic coordinate system and HEALPix projection.  This file is distributed and maintained by LAMBDA
%Copyright          LAMBDA/NASA
%Origin             CDS
%Id                 P/Haslam408
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        1
%Aladin.XLabel      Haslam 408MHz
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-08
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2016-12-20T14:53Z

%ActionName         P-INTEGRAL-14y-17-60keV.hpx
%Description        INTEGRAL/IBIS 14-year 17-60keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/INTEGRAL_14y_17_60
%VerboseDescr       INTEGRAL/IBIS fourteen-year Galactic Hard X-Ray Survey (17-60 keV). The survey covers the Galactic Plane (|b|<17.5deg), at 12' angular resolution. Units of the map are mCrab. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/INTEGRAL/14y/17-60keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.3128
%Aladin.XLabel      INTEGRAL/IBIS 14-year 17-60keV
%Aladin.Tree        Image/X-ray/INTEGRAL
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-16T11:03Z

%ActionName         P-INTEGRAL-17-35keV.hpx
%Description        INTEGRAL/IBIS 9-year 17-35keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/INTEGRAL_17_35
%VerboseDescr       INTEGRAL/IBIS nine-year Galactic Hard X-Ray Survey (17-35 keV). The survey covers the Galactic Plane (|b|<17.5deg), at 12' angular resolution. Units of the map are mCrab. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/INTEGRAL/17-35keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.3128
%Aladin.XLabel      INTEGRAL/IBIS 9-year 17-35keV
%Aladin.Tree        Image/X-ray/INTEGRAL
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-16T10:31Z

%ActionName         P-INTEGRAL-17-60keV.hpx
%Description        INTEGRAL/IBIS 9-year 17-60keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/INTEGRAL_17_60
%VerboseDescr       INTEGRAL/IBIS nine-year Galactic Hard X-Ray Survey (17-60 keV). The survey covers the Galactic Plane (|b|<17.5deg), at 12' angular resolution. Units of the map are mCrab. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/INTEGRAL/17-60keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.3128
%Aladin.XLabel      INTEGRAL/IBIS 9-year 17-60keV
%Aladin.Tree        Image/X-ray/INTEGRAL
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-16T11:10Z

%ActionName         P-INTEGRAL-20-35kev.hpx
%Description        INTEGRAL IBIS 20-35 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Integral/20-35
%VerboseDescr       All public IBIS observations from the Integral Science Data Center (ISDC) in the 20-35 keV energy band.
%Copyright          G. Belanger
%Origin             ESAVO
%Id                 P/INTEGRAL/20-35kev
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/integral/data-publication-credits
%SkyFraction        0.8379
%Aladin.XLabel      INTEGRAL 20-35 keV
%Aladin.Tree        Image/X/INTEGRAL
%Aladin.HpxParam    3 image equatorial png jpeg fits
%Aladin.Date        2016-05-20T08:51Z

%ActionName         P-INTEGRAL-35-65kev.hpx
%Description        INTEGRAL IBIS 35-65 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Integral/35-65
%VerboseDescr       All public IBIS observations from the Integral Science Data Center (ISDC) in the 35-65 keV energy band.
%Copyright          G. Belanger
%Origin             ESAVO
%Id                 P/INTEGRAL/35-65kev
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/integral/data-publication-credits
%SkyFraction        0.8535
%Aladin.XLabel      INTEGRAL 35-65 keV
%Aladin.Tree        Image/X/INTEGRAL
%Aladin.HpxParam    3 image equatorial png jpeg fits
%Aladin.Date        2016-05-19T14:22Z

%ActionName         P-INTEGRAL-35-80keV.hpx
%Description        INTEGRAL/IBIS 9-year 35-80keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551170260  2019/02/26 10:37:40
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/INTEGRAL_35_80
%VerboseDescr       INTEGRAL/IBIS nine-year Galactic Hard X-Ray Survey (35-80 keV). The survey covers the Galactic Plane (|b|<17.5deg), at 12' angular resolution. Units of the map are mCrab. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/INTEGRAL/35-80keV
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.3128
%Aladin.XLabel      INTEGRAL/IBIS 9-year 35-80keV
%Aladin.Tree        Image/X-ray/INTEGRAL
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2019-01-16T10:52Z

%ActionName         P-INTEGRAL-65-100kev.hpx
%Description        INTEGRAL IBIS 65-100 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Integral/65-100
%VerboseDescr       All public IBIS observations from the Integral Science Data Center (ISDC) in the 65-100 keV energy band.
%Copyright          G. Belanger
%Origin             ESAVO
%Id                 P/INTEGRAL/65-100kev
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/integral/data-publication-credits
%SkyFraction        0.8528
%Aladin.XLabel      INTEGRAL 65-100 keV
%Aladin.Tree        Image/X/INTEGRAL
%Aladin.HpxParam    3 image equatorial png jpeg fits
%Aladin.Date        2016-05-19T14:22Z

%ActionName         P-INTEGRAL-color.hpx
%Description        INTEGRAL IBIS color composition (Blue: 20-35 keV; green: 35-65 keV; reg: 65-100 keV)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/Integral/color
%VerboseDescr       All public IBIS observations from the Integral Science Data Center (ISDC).
%Copyright          G. Belanger
%Origin             ESAVO
%Id                 P/INTEGRAL/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cosmos.esa.int/web/integral/data-publication-credits
%SkyFraction        0.9909
%Aladin.XLabel      INTEGRAL-color
%Aladin.Tree        Image/X/INTEGRAL
%Aladin.HpxParam    3 image color equatorial jpeg
%Aladin.Date        2016-05-16T15:50Z

%ActionName         P-INTGAL-35.hpx
%Description        Nine Year INTEGRAL IBIS 17-35 keV Galactic Plan
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/INTGAL/INTGAL35
%VerboseDescr       This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K).
%Copyright          HiPSized & color composition by CDS
%Origin             CDS
%Id                 P/INTGAL/35
%Aladin.Profile     >6.1
%Copyright.Url      http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php
%SkyFraction        0.3108
%Aladin.XLabel      INTGAL 35
%Aladin.Tree        Image/X/INTEGRAL/INTGAL
%Aladin.MenuNumber  01-03-01-01
%Aladin.HpxParam    3 image equatorial png fits
%Aladin.Date        2015-01-12T17:23Z

%ActionName         P-INTGAL-60.hpx
%Description        Nine Year INTEGRAL IBIS 17-60 keV Galactic Plan
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/INTGAL/INTGAL60
%VerboseDescr       This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K).
%Copyright          Space Research Institute (IKI), Moscow, Russia
%Origin             CDS
%Id                 P/INTGAL/60
%Aladin.Profile     >6.1
%Copyright.Url      http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php
%SkyFraction        0.3108
%Aladin.XLabel      INTGAL 60
%Aladin.Tree        Image/X/INTEGRAL/INTGAL
%Aladin.MenuNumber  01-03-01-02
%Aladin.HpxParam    3 image equatorial png fits
%Aladin.Date        2015-01-12T17:28Z

%ActionName         P-INTGAL-80.hpx
%Description        Nine Year INTEGRAL IBIS 35-80 keV Galactic Plan
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/INTGAL/INTGAL80
%VerboseDescr       This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K).
%Copyright          Space Research Institute (IKI), Moscow, Russia
%Origin             CDS
%Id                 P/INTGAL/80
%Aladin.Profile     >6.1
%Copyright.Url      http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php
%SkyFraction        0.3108
%Aladin.XLabel      INTGAL 80
%Aladin.Tree        Image/X/INTEGRAL/INTGAL
%Aladin.MenuNumber  01-03-01-03
%Aladin.HpxParam    3 image equatorial png fits
%Aladin.Date        2015-01-12T17:28Z

%ActionName         P-INTGAL-Color.hpx
%Description        Nine Year INTEGRAL IBIS Galactic Plan Color Composition (35-60-80KeV)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/INTGAL/INTColor
%VerboseDescr       This survey combines the 3 bands of the 9 years of INTEGRAL IBIS surveys described in Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K).
%Copyright          Space Research Institute (IKI), Moscow, Russia
%Origin             CDS
%Id                 P/INTGAL/Color
%Aladin.Profile     >6.1
%Copyright.Url      http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php
%SkyFraction        0.3828
%Aladin.XLabel      INTGAL Color
%Aladin.Tree        Image/X/INTEGRAL/INTGAL
%Aladin.MenuNumber  01-03-01-00
%Aladin.HpxParam    3 image equatorial png jpeg
%Aladin.Date        2015-01-12T17:48Z

%ActionName         P-IPHAS-DR2-halpha.hpx
%Description        IPHAS DR2 halpha
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/IPHAS/DR2/halpha
%VerboseDescr       The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1860 deg2 imaging survey of the Northern Milky Way at red visible wavelengths. It covers Galactic latitudes |b| < 5° and longitudes l = 30-215° in the broad-band r, i and narrow-band H? filters.
%Copyright          IPHAS
%Origin             CDS
%Id                 P/IPHAS/DR2/halpha
%Aladin.Profile     >6.1
%SkyFraction        0.04448
%Aladin.XLabel      IPHAS DR2 halpha
%Aladin.Tree        Image/Optical/IPHAS
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2019-03-16T10:14Z

%ActionName         P-IPHAS-DR2-i.hpx
%Description        IPHAS DR2 i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/IPHAS/DR2/i/CDS_P_IPHAS_DR2_i
%VerboseDescr       The INT/WFC Photometric H-Alpha Survey of the Northen Galactic Plane (IPHAS) is a 1860 deg2 imaging survey of the Northen Milky Way at red visible wavelenghts. It covers Galactic latitude |b| <5 deg and logitudes l = 30-215 deg in the broad-band r, i, and narrow-bnad H alpha filters.
%Copyright          IPHAS
%Origin             CDS
%Id                 P/IPHAS/DR2/i
%Aladin.Profile     >6.1
%SkyFraction        0.04448
%Aladin.XLabel      IPHAS DR2 i
%Aladin.Tree        Image/Optical/IPHAS
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2019-03-13T07:19Z

%ActionName         P-IPHAS-DR2-r.hpx
%Description        IPHAS DR2 r
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/IPHAS/DR2/r/CDS_P_IPHAS_DR2_r
%VerboseDescr       The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1860 deg2 imaging survey of the Northern Milky Way at red visible wavelengths. It covers Galactic latitudes |b| < 5° and longitudes l = 30-215° in the broad-band r, i and narrow-band H? filters.
%Copyright          IPHAS
%Origin             CDS
%Id                 P/IPHAS/DR2/r
%Aladin.Profile     >6.1
%SkyFraction        0.04448
%Aladin.XLabel      IPHAS DR2 r
%Aladin.Tree        Image/Optical/IPHAS
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2019-03-18T10:59Z

%ActionName         P-IRIS-1.hpx
%Description        IRAS-IRIS BAND 1 - 12um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRIS_1
%VerboseDescr       Improved Reprocessing of the IRAS Survey (IRIS) (Band 1 - 12 microns) at the 3.8' resolution. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRIS/1
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      IRIS band 1 - 12um
%Aladin.Tree        Image/Infrared/IRIS
%Aladin.MenuNumber  04-02-02
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-07-16T15:28Z

%ActionName         P-IRIS-2.hpx
%Description        IRAS-IRIS BAND 2 - 25um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRIS_2
%VerboseDescr       Improved Reprocessing of the IRAS Survey (IRIS) (Band 2 - 25 microns) at the 3.8' resolution. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRIS/2
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      IRIS band 2 - 25um
%Aladin.Tree        Image/Infrared/IRIS
%Aladin.MenuNumber  04-02-03
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-07-16T15:35Z

%ActionName         P-IRIS-3.hpx
%Description        IRAS-IRIS BAND 3 - 60um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRIS_3
%VerboseDescr       Improved Reprocessing of the IRAS Survey (IRIS) (Band 3 - 60 microns) at the 4.0' resolution. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRIS/3
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      IRIS band 3 - 60um
%Aladin.Tree        Image/Infrared/IRIS
%Aladin.MenuNumber  04-02-04
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-07-16T15:41Z

%ActionName         P-IRIS-4.hpx
%Description        IRAS-IRIS BAND 4 - 100um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1456391319  2016/02/25 11:08:39
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRIS_4
%VerboseDescr       Improved Reprocessing of the IRAS Survey (IRIS) (Band 4 - 100 microns) at the 4.3' resolution. Units: MJy/sr\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRIS/4
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      IRIS band 4 - 100um
%Aladin.Tree        Image/Infrared/IRIS
%Aladin.MenuNumber  04-02-05
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-07-16T15:46Z

%ActionName         P-IRIS-color.hpx
%Description        IRAS-IRIS HEALPix survey, color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-IRIS-color_0.hpx availability=0
%SeeAction          P-IRIS-color_1.hpx availability=11
%SeeAction          P-IRIS-color_2.hpx availability=0
%SeeAction          P-IRIS-color_3.hpx availability=0
%SeeAction          P-IRIS-color_4.hpx availability=9999
%SeeAction          P-IRIS-color_5.hpx availability=10
%VerboseDescr       The Infrared Astronomical Satellite (IRAS) had a tremendous impact on many areas of modern astrophysics. In particular it revealed the ubiquity of infrared cirrus that are a spectacular manifestation of the interstellar medium complexity but also an important foreground for observational cosmology. With the forthcoming Planck satellite there is a need for all-sky complementary data sets with arcminute resolution that can bring informations on specific foreground emissions that contaminate the Cosmic Microwave Background radiation. With its ~4' resolution matching perfectly the high-frequency bands of Planck, IRAS is a natural data set to study the variations of dust properties at all scales. But the latest version of the images delivered by the IRAS team (the ISSA plates) suffers from calibration, zero level and striping problems that can preclude its use, especially at 12 and 25 micron. In this paper we present how we proceeded to solve each of these problems and enhance significantly the general quality of the ISSA plates in the four bands (12, 25, 60 and 100 microns). This new generation of IRAS images, called IRIS, benefits from a better zodiacal light subtraction, from a calibration and zero level compatible with DIRBE, and from a better destriping. At 100 micron the IRIS product is also a significant improvement from the Schlegel et al. (1998) maps. IRIS keeps the full ISSA resolution, it includes well calibrated point sources and the diffuse emission calibration at scales smaller than 1 degree was corrected for the variation of the IRAS detector responsivity with scale and brightness. The uncertainty on the IRIS calibration and zero level are dominated by the uncertainty on the DIRBE calibration and on the accuracy of the zodiacal light model.
%Copyright          Healpixed by CDS
%Origin             CDS
%Id                 P/IRIS/color
%Aladin.Profile     >6.1
%Copyright.Url      http://irsa.ipac.caltech.edu/data/IRIS/
%SkyFraction        1
%Aladin.XLabel      IRIS color
%Aladin.Tree        Image/Infrared/IRIS
%Aladin.MenuNumber  04-02-01 lite
%Aladin.HpxParam    3 image color galactic jpeg
%Aladin.Date        2010-06-09T06:33Z

%ActionName         P-IRTS-250.hpx
%Description        IRTS 250um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRTS_250
%VerboseDescr       The Infrared Telescope in Space (IRTS) - Images obtained with the IRTS/FIRP instrument at 250 mic, at a resolution of 0.5 deg. Units: W/m2/sr/Hz\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRTS/250
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.03019
%Aladin.XLabel      IRTS 250um
%Aladin.Tree        Image/Radio/IRTS
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2015-01-15T17:12Z

%ActionName         P-IRTS-400.hpx
%Description        IRTS 400um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRTS_400
%VerboseDescr       The Infrared Telescope in Space (IRTS)- Images obtained with the IRTS/FIRP instrument at 400 mic, at a resolution of 0.5 deg. Units: W/m2/sr/Hz\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRTS/400
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.004817
%Aladin.XLabel      IRTS 400um
%Aladin.Tree        Image/Radio/IRTS
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2015-01-15T17:14Z

%ActionName         P-IRTS-700.hpx
%Description        IRTS 700um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/IRTS_700
%VerboseDescr       The Infrared Telescope in Space (IRTS)- Images obtained with the IRTS/FIRP instrument at 700 mic, at a resolution of 0.5 deg. Units: W/m2/sr/Hz\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/IRTS/700
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05209
%Aladin.XLabel      IRTS 700um
%Aladin.Tree        Image/Radio/IRTS
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2015-01-15T17:18Z

%ActionName         P-ISO-CAM.hpx
%Description        ISOCAM
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1472890029  2016/09/03 10:07:09
%Url                http://skies.esac.esa.int/ISO/CAM
%VerboseDescr       All public ISOCAM observations from the ISO Data Archive.
%Copyright          ESA/IDA
%Origin             ESAVO
%Id                 P/ISO/CAM
%Aladin.Profile     >6.1
%Copyright.Url      http://iso.esac.esa.int/ida/
%SkyFraction        0.004086
%Aladin.XLabel      ISOCAM
%Aladin.Tree        Image/Infrared/ISO
%Aladin.HpxParam    8 image equatorial jpeg png fits
%Aladin.Date        2016-03-17T12:35Z

%ActionName         P-ISOPHOT-170.hpx
%Description        The ISOPHOT 170um Serendipity Survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ISO/ISOPHOT
%VerboseDescr       The 170 micron far-infrared slew data of the ISOPHOT Serendipity Survey (ISOSS) has been assembled to a sky atlas with about 15% sky coverage. The redundant information of the brightnesss at slew crossings has been used to globally rescale and homogenize the slew brightnesses, leading to significantly increased photometric accuracy and reproducibility as well as the homogeneity of the maps. The corrected slew data were remapped with a constant grid size of 22.4arcsec onto 124 maps in galactic coordinates - (Stickel et al., 2007)
%Copyright          Stickel et al., 2007 - HiPSed by CDS
%Origin             CDS
%Id                 P/ISOPHOT/170
%Aladin.Profile     >6.1
%Copyright.Url      http://cdsarc.u-strasbg.fr/viz-bin/Cat?J/A%2bA/466/1205
%SkyFraction        0.3096
%Aladin.XLabel      ISOPHOT 170 um
%Aladin.Tree        Image/Infrared/ISO
%Aladin.MenuNumber  04-xx
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2014-12-05T13:45Z

%ActionName         P-Iapetus-Cassini-PIA18436.hpx
%Description        Iapetus Cassini PIA18436
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Iapetus_Cassini-PIA18436
%VerboseDescr       This set of global, color mosaics of Saturn's moon Iapetus was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system. These are the first global color maps of these moons produced from the Cassini data. The colors shown in these global mosaics are enhanced, or broader, relative to human vision, extending into the ultraviolet and infrared range. Resolution on Iapetus in the maps is 400 meters per pixel. Image selection, radiometric calibration, geographic registration and photometric correction, as well as mosaic selection and assembly were performed by Paul Schenk at the Lunar and Planetary Institute. Original image planning and targeting for Saturn's icy moons were performed by Tilman Denk (Frei Universitat, Berlin) and Paul Helfenstein (Cornell University, Ithaca, New York). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.
%Copyright          JPL/PhotoJournal
%Origin             CDS
%Id                 P/Iapetus/Cassini-PIA18436
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Iapetus/Cassini-PIA18436
%Aladin.Tree        Solar system/Saturn/Iapetus
%Aladin.HpxParam    3 image color iapetus jpeg
%Aladin.Date        2018-01-24T14:14Z

%ActionName         P-Io-Galileo-SSI-1km.hpx
%Description        Io Galileo-SSI-1km
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Io_Galileo-SSI-1km
%VerboseDescr       This basemap of Jupiter?s moon Io was produced by combining the best images from both the Voyager 1 and Galileo Missions. Although the subjovian hemisphere of Io was poorly seen by Galileo, superbly detailed Voyager 1 images cover longitudes from 240?W to 40?W and the nearby southern latitudes. A monochrome mosaic of the highest resolution images from both Galileo and Voyager 1 was assembled that includes 29 Voyager 1 images with spatial resolutions sometimes exceeding the 1 km/pixel scale of the final mosaic. Because this mosaic is made up of images taken at various local times of day, care must be taken to note the solar illumination direction when deciding whether topographic features display positive or negative relief. In general, the illumination is from the west over longitudes 40 to 270 W, and from the east over longitudes 270 W to 40 W. Color information was later superimposed from Galileo low phase angle violet, green, and near-infrared (756 nanometer wavelength) images. The Galileo Solid-State Imaging (SSI) camera?s silicon charge-coupled device (CCD) was sensitive to longer wavelengths than the vidicon cameras of Voyager, so that distinctions between red and yellow hues can be more easily discerned. The ?true? colors that would be visible to the eye are similar but much more muted than shown here. Image resolutions range from 1 to 10 km/pixel along the equator, with the poorest coverage centered on longitude 50 W
%Copyright          Public domain
%Origin             CDS
%Id                 P/Io/Galileo-SSI-1km
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Io/Galileo-SSI-1km
%Aladin.Tree        Solar system/Jupiter/Io
%Aladin.HpxParam    3 image color io
%Aladin.Date        2018-01-14T18:34Z

%ActionName         P-JPSPR1.hpx
%Description        JPS-PR1 850um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/pub/arXiv.1704.02982v1/JPSPR1
%VerboseDescr       The first data release of the James Clerk Maxwell Telescope (JCMT) Plane Survey (JPS), the JPS Public Release 1 (JPSPR1). JPS is an 850-um continuum survey of six fields in the northern inner Galactic Plane in a longitude range of l=7-63, made with the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2). This first data release consists of emission maps of the six JPS regions with an average pixel-to-pixel noise of 7.19 mJy beam^-1, when smoothed over the beam, and a compact-source catalogue containing 7,813 sources. The 95 per cent completeness limits of the catalogue are estimated at 0.04 Jy beam^-1 and 0.3 Jy for the peak and integrated flux densities, respectively. The emission contained in the compact-source catalogue is 42 +- 5 per cent of the total and, apart from the large-scale (greater than 8') emission, there is excellent correspondence with features in the 500-um Herschel maps.
%Copyright          CANFAR
%Origin             CDS
%Id                 P/JPSPR1
%Aladin.Profile     >6.1
%SkyFraction        0.002219
%Aladin.XLabel      JPS-PR1
%Aladin.Tree        Image/Infrared
%Aladin.HpxParam    8 image equatorial png fits
%Aladin.Date        2017-05-03T14:20Z

%ActionName         P-Jupiter-PIA07782.hpx
%Description        Jupiter PIA07782
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Jupiter_PIA07782
%Origin             CDS
%Id                 P/Jupiter/PIA07782
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Jupiter/PIA07782
%Aladin.Tree        Solar system/Jupiter
%Aladin.HpxParam    3 image color jupiter jpeg
%Aladin.Date        2018-01-13T19:01Z

%ActionName         P-LAB.hpx
%Description        Leiden/Argentine/Bonn (LAB) Galactic HI survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1461076880  2016/04/19 16:41:20
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/LAB_NH
%VerboseDescr       21-cm emission from Galactic neutral hydrogen over the entire sky. Observations made using the Dwingeloo 25-m telescope. The effective resolution of the map is 40'. Units: H/cm2\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/LAB
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      Dwingeloo LAB NH
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.MenuNumber  06-04
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-11-26T14:34Z

%ActionName         P-MAIPU-MU.hpx
%Description        MAIPU-MU 45 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/MAIPU-MU
%VerboseDescr       45 MHz continuum survey, made with the 45-MHz array of the University of Chile at the Maipu Radio Astronomy Observatory (south of declination +19.1 degrees)and the circular filled array of the Japanese Middle and Upper Atmosphere Radar (declination range between +5 degrees and +65 degrees). The angular resolution is approximately 5 degrees. Units: KTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/MAIPU-MU
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.9635
%Aladin.XLabel      MAIPU-MU 45 MHz
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-07T09:56Z

%ActionName         P-MAMA-ColorEJ.hpx
%Description        MAMA color composition (posse,srcj)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/MAMA/CDS_P_MAMA_color_posse_srcj
%VerboseDescr       During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band.
%Copyright          Observatoire de Paris
%Origin             CDS
%Id                 P/MAMA/ColorEJ
%Aladin.Profile     >6.1
%Copyright.Url      https://www.obspm.fr/mentions-legales.html?lang=en
%SkyFraction        0.3012
%Aladin.XLabel      MAMA Color
%Aladin.Tree        Image/Optical/MAMA
%Aladin.HpxParam    10 image color equatorial png
%Aladin.Date        2017-12-20T16:11Z

%ActionName         P-MAMA-posse.hpx
%Description        MAMA posse
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/MAMA/CDS_P_MAMA_posse
%VerboseDescr       During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band.
%Copyright          Observatoire de Paris
%Origin             CDS
%Id                 P/MAMA/posse
%Aladin.Profile     >6.1
%Copyright.Url      https://www.obspm.fr/mentions-legales.html?lang=en
%SkyFraction        0.3012
%Aladin.XLabel      MAMA posse
%Aladin.Tree        Image/Optical/MAMA
%Aladin.HpxParam    10 image equatorial png fits
%Aladin.Date        2016-09-12T21:38Z

%ActionName         P-MAMA-srcj.hpx
%Description        MAMA srcj
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/MAMA/CDS_P_MAMA_srcj
%VerboseDescr       During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band.
%Copyright          Observatoire de Paris
%Origin             CDS
%Id                 P/MAMA/srcj
%Aladin.Profile     >6.1
%Copyright.Url      https://www.obspm.fr/mentions-legales.html?lang=en
%SkyFraction        0.5241
%Aladin.XLabel      MAMA srcj
%Aladin.Tree        Image/Optical/MAMA
%Aladin.HpxParam    10 image equatorial png fits
%Aladin.Date        2016-06-30T05:19Z

%ActionName         P-MAXI-GSC.hpx
%Description        MAXI GSC All sky image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/maxi_gsc_sum
%VerboseDescr       MAXI GSC All sky pserudo-color image from 2009 to 2015 March
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/MAXI-GSC
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/maxi
%Aladin.XLabel      MAXI
%Aladin.Tree        Image/X/MAXI
%Aladin.HpxParam    color equatorial png
%Aladin.Date        2015/03/30 15:08:54

%ActionName         P-MAXI-SSC.hpx
%Description        MAXI SSC All sky image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/maxi_ssc_sum
%VerboseDescr       MAXI SSC All sky pserudo-color image from 2009 to 2015 March
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/MAXI-SSC
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/maxi
%SkyFraction        1
%Aladin.XLabel      MAXI
%Aladin.Tree        Image/X/MAXI
%Aladin.HpxParam    color equatorial png
%Aladin.Date        2015/03/30 15:08:54

%ActionName         P-MITEoR.hpx
%Description        MITEoR 150 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/MITEoR
%VerboseDescr       Northern sky survey from 128 to 175 MHz using the MIT Epoch of Reionization (MITEoR) experiment, at an angular resolution of approximately 2 degrees. Units: mKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/MITEoR
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.4284
%Aladin.XLabel      MITEoR 150 MHz
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-07T08:35Z

%ActionName         P-MaNGA.hpx
%Description        MaNGA LOGCUBE data cube
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/MaNGA
%VerboseDescr       MaNGA (Mapping Nearby Galaxies at APO) is the newest survey component of the Sloan Digital Sky Survey. Its goal is to map the detailed composition and kinematic structure of 10,000 nearby galaxies. MaNGA uses integral field unit (IFU) spectroscopy to measure spectra for hundreds of points within each galaxy. The 3-D data cubes that constitute the final MaNGA data products are constructed from a few tens to a few thousands of individual spectra that have been combined onto a regular grid. The LOGCUBE data cube has logarithmic wavelength sampling from log10(lambda/Angstroms)=3.5589 to 4.0151 (NWAVE=4563 spectral elements), and 0.5 arcsec spatial pixels (spaxels) for a total size of NX x NY x NWAVE pixels; LINCUBE is the same, except it has linear wavelength sampling from from 3622.0 to 10353.0 Angstroms (NWAVE=6732 spectral elements).
%Copyright          Sloan Digital Sky Survey
%Origin             CDS
%Id                 P/MaNGA
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/dr13/manga/manga-data/data-access/
%SkyFraction        4.219E-6
%Aladin.XLabel      MaNGA
%Aladin.Tree        Cube
%Aladin.HpxParam    12 cube equatorial png fits
%Aladin.Date        2016-12-15T16:07Z

%ActionName         P-Mars-Express286545.hpx
%Description        Mapping Mars (Mars Express)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_Express286545
%VerboseDescr       The latest Mars image mosaic as seen through the lens of the High Resolution Stereo Camera on ESA?s Mars Express. The mosaic comprises 2702 individual swaths of the martian surface, up to and including the spacecraft?s 10 821st orbit of the planet, which it completed on 30 June 2012. At this time, 87.8% of the surface had been mapped at any resolution, with 61.5% mapped at a resolution of 20 m per pixel or better.
%Copyright          ESA/DLR/FU Berlin (G. Neukum)
%Origin             CDS
%Id                 P/Mars/Express286545
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mars/Express286545
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    3 image mars jpeg
%Aladin.Date        2018-01-14T17:21Z

%ActionName         P-Mars-MGS-MOLA-DEM.hpx
%Description        Mars MGS MOLA Elevation Model 463m (MEGDR)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/Mars_MGS_MOLA_DEM
%VerboseDescr       Mars MGS MOLA Digital Elevation Model (DEM) is based on data from the Mars Orbiter Laser Altimeter (MOLA; Smith and others, 2001), an instrument on NASA?s Mars Global Surveyor (MGS) spacecraft (Albee and others, 2001). The DEM represents more than 600 million measurements gathered between 1999 and 2001, adjusted for consistency (Neumann and others, 2001, 2003) and converted to planetary radii. These have been converted to elevations above the areoid as determined from a Martian gravity field solution GMM-2B (Lemoine and others, 2001), truncated to degree and order 50, and oriented according to current standards. The average accuracy of each point is originally ~100 meters in horizontal position and ~1 meter in radius (Neumann and others, 2001). However, the total elevation uncertainty is at least ±3 m due to the global error in the areoid (±1.8 meters according to Lemoine and others [2001]) and regional uncertainties in its shape (G.A. Neumann, written commun., 2002).
%Copyright          Public domain, Please cite authors
%Origin             CDS
%Id                 P/Mars/MGS-MOLA-DEM
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Mars MGS-MOLA-DEM
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    4 image mars jpeg fits
%Aladin.Date        2017-09-08T11:42Z

%ActionName         P-Mars-MGS-TES-Dust.hpx
%Description        Mars MGS TES Dust
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_MGS-TES-Dust
%VerboseDescr       Mars Surface Dust Cover Index. NASA MGS/TES. 16 ppd/3.5km.
%Copyright          Arizona State University
%Origin             CDS
%Id                 P/Mars/MGS-TES-Dust
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mars/MGS-TES-Dust
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    3 image color mars jpeg
%Aladin.Date        2018-01-27T17:38Z

%ActionName         P-Mars-MOLA-color.hpx
%Description        Mars MOLA Shaded Relief / Colorised Elevation
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/Mars_MOLA
%Origin             CDS
%Id                 P/Mars/MOLA-color
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Mars MOLA
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    5 image color mars jpeg
%Aladin.Date        2017-09-10T15:46Z

%ActionName         P-Mars-Pan-PIA20284.hpx
%Description        Mars Panorama PIA20284
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_Pan-PIA20284
%VerboseDescr       This view of the downwind face of "Namib Dune" on Mars covers 360 degrees, including a portion of Mount Sharp on the horizon. The site is part of the dark-sand "Bagnold Dunes" field along the northwestern flank of Mount Sharp. Images taken from orbit indicate that dunes in the Bagnold field move as much as about 3 feet (1 meter) per Earth year. The component images of this scene were taken on Dec. 18, 2015, by the Mast Camera (Mastcam) on NASA's Curiosity Mars rover during the 1,197th Martian day, or sol, of the rover's work on Mars.
%Copyright          NASA/JPL-Caltech/MSSS
%Origin             CDS
%Id                 P/Mars/Pan-PIA20284
%Aladin.Profile     >6.1 beta
%Copyright.Url      https://photojournal.jpl.nasa.gov/catalog/PIA20284
%SkyFraction        0.8385
%Aladin.XLabel      P/Mars/Pan-PIA20284
%Aladin.Tree        Solar system/Mars/Panorama
%Aladin.HpxParam    3 image color MarsPanorama jpeg
%Aladin.Date        2018-01-13T21:27Z

%ActionName         P-Mars-Pan-Stimson.hpx
%Description        Mars Stimson panorama
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_Pan-Stimson
%VerboseDescr       360-degree panorama acquired by the Mast Camera (Mastcam) on NASA's Curiosity Mars rover on April 4, 2016, as part of long-term campaign to document the context and details of the geology and landforms along Curiosity's traverse since landing in August 2012
%Copyright          NASA/JPL-Caltech/MSSS
%Origin             CDS
%Id                 P/Mars/Pan-Stimson
%Aladin.Profile     >6.1 beta
%Copyright.Url      https://photojournal.jpl.nasa.gov/catalog/PIA20332
%SkyFraction        0.6875
%Aladin.XLabel      Mars_Stimson
%Aladin.Tree        Solar system/Mars/Panorama
%Aladin.MenuNumber  ZZ
%Aladin.HpxParam    4 image color mars-panstimson jpg
%Aladin.Date        2017-06-26T08:03Z

%ActionName         P-Mars-TES-Albedo.hpx
%Description        Mars TES Albedo
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_TES-Albedo
%VerboseDescr       Mars surface albedo. MGS/TES. 8 ppd/7.5km.
%Copyright          Arizona State University
%Origin             CDS
%Id                 P/Mars/TES-Albedo
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mars/TES-Albedo
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    3 image color mars jpeg
%Aladin.Date        2018-01-27T17:48Z

%ActionName         P-Mars-TES-Thermal-Inertia.hpx
%Description        Mars TES Thermal Inertia
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_TES-Thermal-Inertia
%VerboseDescr       Mars colorized thermal inertia from NASA MGS/TES. 8 ppd/7.5km.
%Copyright          Arizona State University
%Origin             CDS
%Id                 P/Mars/TES-Thermal-Inertia
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9635
%Aladin.XLabel      P/Mars/TES-Thermal-Inertia
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    3 image color mars jpeg
%Aladin.Date        2018-01-27T18:06Z

%ActionName         P-Mars-THEMIS-Day-100m-v12.hpx
%Description        Mars THEMIS-Day-100m-v12
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_THEMIS-Day-100m-v12
%VerboseDescr       Daytime thermal infrared (12.57um) mosaic. 593 ppd/99m. NASA Mars Odyssey/THEMIS (version 12)
%Copyright          Arizona State University, intermediate FITS by Chiara Marmo
%Origin             CDS
%Id                 P/Mars/THEMIS-Day-100m-v12
%Aladin.Profile     >6.1 beta
%SkyFraction        0.999
%Aladin.XLabel      P/Mars/THEMIS-Day-100m-v12
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    7 image mars jpeg fits
%Aladin.Date        2019-01-08T10:48Z

%ActionName         P-Mars-THEMIS-IR-Night-100m-v14.hpx
%Description        Mars THEMIS-IR-Night-100m-v14
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_THEMIS-IR-Night-100m-v14
%VerboseDescr       Mars THEMIS nighttime thermal infrared (12.57um) mosaic. 593 ppd/100m. NASA Mars Odyssey/THEMIS
%Copyright          Arizona State University - Intermediate FITS file by Chiara Marmo
%Origin             CDS
%Id                 P/Mars/THEMIS-IR-Night-100m-v14
%Aladin.Profile     >6.1 beta
%SkyFraction        0.8511
%Aladin.XLabel      P/Mars/THEMIS-IR-Night-100m-v14
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    7 image mars jpeg fits
%Aladin.Date        2019-01-08T09:16Z

%ActionName         P-Mars-THEMIS-color.hpx
%Description        Mars THEMIS Day IR Global Mosaic 100m v12
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/Mars_THEMIS
%VerboseDescr       Mars THEMIS Day IR Global Mosaic 100m v12 represents the Thermal Emission Imaging System (THEMIS) -daytime infrared (IR) 100 meter/pixel mosaic (version 12) released in the summer of 2014 by Arizona State University. Values represent only a visual representation of day-time temperatures. The original values have been stretched and blended to make a more seamless mosaic. It has been hipsilized by CDS from the JPEG cartesian global map.
%Copyright          Public domain
%Origin             CDS
%Id                 P/Mars/THEMIS-color
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Mars THEMIS Day IR Global Mosaic
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    5 image color mars jpeg
%Aladin.Date        2017-09-10T15:16Z

%ActionName         P-Mars-Viking-MDIM21-color.hpx
%Description        Mars Viking-MDIM21-color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/Mars_Viking_MDIM21
%Copyright          USGS (https://astrogeology.usgs.gov/), intermediate FITS by Chiara Marmo
%Origin             CDS
%Id                 P/Mars/Viking-MDIM21-color
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Mars Viking-MDIM21-color
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    5 image color mars jpeg
%Aladin.Date        2017-11-13T13:18Z

%ActionName         P-Mars-mola-roughness.hpx
%Description        Mars mola-roughness
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mars_mola-roughness
%VerboseDescr       Mars MOLA Vertical Roughness. Krevalsky & Head vertical roughness. Red, green and blue composite from roughness at 0.6 km, 2.4 km, and 9.2 km baselines. 8 ppd/7.5km
%Origin             CDS
%Id                 P/Mars/mola-roughness
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mars/mola-roughness
%Aladin.Tree        Solar system/Mars
%Aladin.HpxParam    3 image color Mars jpeg
%Aladin.Date        2018-01-27T17:29Z

%ActionName         P-Mellinger-color.hpx
%Description        Mellinger color optical survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-Mellinger-color_0.hpx availability=0
%SeeAction          P-Mellinger-color_1.hpx availability=0
%SeeAction          P-Mellinger-color_2.hpx availability=0
%VerboseDescr       Using a portable low-cost CCD camera system, 70 fields (each covering 40deg×27deg) were imaged over a time span of 22 months from dark-sky locations in South Africa, Texas, and Michigan. The fields were photometrically calibrated against standard catalog stars. Using sky background data from the Pioneer 10 and 11 space probes, gradients resulting from artificial light pollution, airglow, and zodiacal light were eliminated, while the large-scale galactic and extragalactic background resulting from unresolved sources was preserved. The 648 megapixel image is a valuable educational tool, being able to fully utilize the resolution and dynamic range of modern full-dome planetarium projection systems.
%Copyright          Copyright 2000-2017 Axel Mellinger. All rights reserved.
%Origin             CDS
%Id                 P/Mellinger/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.milkywaysky.com/
%SkyFraction        1
%Aladin.XLabel      Mellinger color
%Aladin.Tree        Image/Optical
%Aladin.MenuNumber  03-03 lite
%Aladin.HpxParam    4 image color galactic jpeg
%Aladin.Date        2014-12-09T09:44Z

%ActionName         P-Mercury-MESSENGER-MDIS-LOI-166m.hpx
%Description        Mercury MESSENGER-MDIS-LOI-166m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mercury_MESSENGER-MDIS-LOI-166m
%VerboseDescr       The Map Projected Low-Incidence Angle Basemap RDR (LOI) data set consists of a global monochrome map of reflectance at a resolution of 256 pixels per degree (~166 m/p). Each original map tile, defined geographically in the same manner as for BDRs, contains a single band that merges NAC and WAC 750-nm images. This edition, version 1, was released May 13, 2016 to the Johns Hopkins Applied Physics Laboratory MESSENGER Team website. The original LOI mosaic was released at end of mission, is compiled in part based on images taken as a part of the global low-incidence angle imaging campaign but also includes any NAC or WAC 750-nm images from any campaign that best fit the intended illumination geometry, i.e., low emission angle and incidence angle near 45°. It is controlled and projected onto a global digital elevation model. It uses a Kasseleinin-Shkuratov photometric model, whose parameters are the same for any given wavelength band across all MESSENGER end-of-mission map data products. This mosaic contains data acquired by the MErcury Surface, Space ENvironment, GEochemistry and Ranging (MESSENGER) Mercury Dual Imaging System (MDIS) instrument.
%Copyright          Planetary Data System, from USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Mercury/MESSENGER-MDIS-LOI-166m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mercury/MESSENGER-MDIS-LOI-166m
%Aladin.Tree        Solar system/Mercury
%Aladin.HpxParam    5 image color mercury jpeg
%Aladin.Date        2018-01-21T16:31Z

%ActionName         P-Mimas-Cassini-PIA17214.hpx
%Description        Mimas Cassini PIA17214
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Mimas_Cassini-PIA17214
%VerboseDescr       This global map of Saturn's moon Mimas was created using images taken during Cassini spacecraft flybys. The moon's large, distinguishing crater, Herschel, is seen on the map at left. The map is an equidistant (simple cylindrical) projection and has a scale of 710 feet (216 meters) per pixel at the equator. The mean radius of Mimas used for projection of this map is 123.2 miles (198.2 kilometers). The resolution of the map is 16 pixels per degree. This product is an update to the map released in August 2012 (see PIA14926). The update includes new images for almost half of the moon's surface, with new images from two close flybys, in Nov. 2016 and Feb. 2017. The moon's western hemisphere, south pole and parts of the eastern hemisphere received updates in this version. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.
%Copyright          JPL/Photojournal
%Origin             CDS
%Id                 P/Mimas/Cassini-PIA17214
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Mimas/Cassini-PIA17214
%Aladin.Tree        Solar system/Saturn/Mimas
%Aladin.HpxParam    3 image color mimas jpeg
%Aladin.Date        2018-01-24T12:05Z

%ActionName         P-Miranda-Voyager.hpx
%Description        Miranda Voyager
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Miranda_Voyager
%VerboseDescr       Miranda Uranus satellite map mosaicked with Voyager imagery by USGS
%Copyright          Caltech/JPL/NASA
%Origin             CDS
%Id                 P/Miranda/Voyager
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Miranda/Voyager
%Aladin.Tree        Solar system/Uranus/Miranda
%Aladin.HpxParam    3 image color miranda jpeg
%Aladin.Date        2018-01-31T06:36Z

%ActionName         P-Moon-Clementine-750nm-118m.hpx
%Description        Moon Clementine-750nm-118m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Moon_Clementine-750nm-118m
%VerboseDescr       The Clementine Ultraviolet/Visible (UVVIS) Version 2 mosaic is a grayscale data set representing the albedo (brightness of the lunar surface) as measured at the 750 nanometer (nm) wavelength by the UVVIS camera (Lee 2009). In late 2008, a revised 750nm mosaic (v. 2.0) was created at USGS to refine the locations of component images by using the latest geodetic control and projecting onto a topographic model of the lunar surface (Archinal 2006). The base map was radiometrically and geometrically controlled, photometrically modeled global image mosaic compiled using more than 43,000 images from the 750nm filter observations.
%Copyright          Public domain
%Origin             CDS
%Id                 P/Moon/Clementine-750nm-118m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Moon/Clementine-750nm-118m
%Aladin.Tree        Solar system/Earth/Moon
%Aladin.HpxParam    5 image color moon
%Aladin.Date        2018-01-21T13:41Z

%ActionName         P-Moon-JSC2007e045375.hpx
%Description        Apollo surface panorama JSC2007e045375
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Moon_pan1
%VerboseDescr       Apollo 11 Landing Site - Cat's Paw Hills (JSC2007e045375)
%Copyright          https://www.lpi.usra.edu/resources/apollopanoramas/pans/?pan=JSC2007e045375
%Origin             CDS
%Id                 P/Moon/JSC2007e045375
%Aladin.Profile     >6.1 beta
%SkyFraction        0.375
%Aladin.XLabel      P/Moon/JSC2007e045375
%Aladin.Tree        Solar system/Earth/Moon/Panorama
%Aladin.HpxParam    3 image color moon-panJSC2007e045375 jpeg
%Aladin.Date        2018-11-22T13:58Z

%ActionName         P-Moon-Kaguya-Evening-V04-474m.hpx
%Description        Moon Kaguya-Evening-V04-474m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Moon_Kaguya-Evening-V04-474m
%VerboseDescr       This near-global mosaic was generated using data from the SELenological and Engineering Explorer (SELENE) ?Kaguya? Terrain Camera (TC) instrument. TC source data originated as map-projected tiles at ~10 m/pixel spatial resolution. The Japan Aerospace Exploration Agency (JAXA) launched the Selenological and Engineering Explorer (SELENE, also called ?Kaguya?) spacecraft to the Moon in September 2007. The mission concluded June 10, 2009 when the spacecraft was intentionally crashed onto the lunar surface. Subsequent data collection and mapping efforts resulted in ?the largest lunar exploration project since the Apollo program? (Haruyama, 2008). The high-performance optical Terrain Camera (TC), a 10-meter spatial resolution stereo-camera, was part of the Lunar Imager/Spectrometer (LISM) instrument suite (Kato, 2007), along with the Multi-band Imager and Spectral Profiler.
%Copyright          JAXA
%Origin             CDS
%Id                 P/Moon/Kaguya-Evening-V04-474m
%Aladin.Profile     >6.1 beta
%Copyright.Url      http://jda.jaxa.jp/en/service.php
%SkyFraction        1
%Aladin.XLabel      P/Moon/Kaguya-Evening-V04-474m
%Aladin.Tree        Solar system/Earth/Moon
%Aladin.HpxParam    3 image color moon png
%Aladin.Date        2017-11-26T14:27Z

%ActionName         P-Moon-LROC-WAC-100m.hpx
%Description        Moon Lunar Reconnaissance Orbiter WAC Global Morphologic Map
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Moon_LROC-WAC-100m
%VerboseDescr       The WAC global mosaic is comprised of over 15,000 images acquired between November 2009 and February 2011. The WAC maps the whole Moon in one month, however the solar incidence angle at the equator changes about 28? from the beginning to the end of the month. To even out the incidence angle variations, the mosaic is comprised of data collected over three periods (1/20/2010 to 1/28/2010, 5/30/2010 to 6/6/2010, 7/24/2010 to 7/31/2010) (Table 1). Some gores were filled with data taken at other times. The non-polar images were map projected onto the GLD100 (WAC derived 100m/pixel DTM) while polar images were map projected on the LOLA shape model (80? to 90? N/S) and the GLD100 (60? to 80? N/S). Accurate positioning of each WAC image was ensured using ephemeris provided by the LOLA and GRAIL team and an improved camera geometry model (Speyerer, E.J. et al, 2014, Pre-flight and On-orbit Geometric Calibration of the Lunar Reconnaissance Orbiter Camera). To reduce brightness discrepancies across image boundaries, all images were corrected to a common photometric geometry using a Hapke model (Sato, H. et al, 2014, Resolved Hapke parameter maps of the Moon). This mosaic uses only the 643 nm band of the WAC. This HiPS has been created based on 100m resolution WAC Global Morphologic map by
%Copyright          Arizona State University
%Origin             CDS
%Id                 P/Moon/LROC-WAC-100m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Moon/LROC-WAC-100m
%Aladin.Tree        Solar system/Earth/Moon
%Aladin.HpxParam    6 image color moon jpeg
%Aladin.Date        2018-02-06T16:26Z

%ActionName         P-Moon-LROC-WAC-GLD100-118m.hpx
%Description        Moon LROC WAC GLD100 118m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Moon_LROC-WAC-GLD100-118m
%VerboseDescr       Color hillshade of the original WAC GLD100 stereo DTM. This color scheme is used for the upcoming Lunar WAC mosaic and Topographic maps (with Nomenclature) produced by the USGS. For outreach and graphical purposes. Using the GLD100 topography, a color relief was created using Global Mapper and exported to a GeoTiff. This was brought back into ISIS for use in Map-a-Planet 2. Pixels do not contain any of the original explicit elevation information. The colorized shaded-relief represents approximate elevations based on the original topographic data.
%Copyright          USGS Astrogeology Science Center from Arizona State University
%Origin             CDS
%Id                 P/Moon/LROC-WAC-GLD100-118m
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9863
%Aladin.XLabel      P/Moon/LROC-WAC-GLD100-118m
%Aladin.Tree        Solar system/Earth/Moon
%Aladin.HpxParam    5 image color moon jpeg
%Aladin.Date        2018-02-06T21:19Z

%ActionName         P-NEOWISER-Color.hpx
%Description        NEOWISER color  Red (W2) , Blue (W1)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/NEOWISER/W1W2
%VerboseDescr       The NEOWISE project is the asteroid-hunting portion of the Wide-field Infrared Survey Explorer (WISE) mission. Funded by NASA's Planetary Science Division, NEOWISE harvests measurements of asteroids and comets from the WISE images and provides a rich archive for searching WISE data for solar system objects. Here we update our full-depth coadds by folding in the most recently published year of W1/W2 exposures released by NEOWISER. These new single-frame data were acquired between 2015 December 13 and 2016 December 13, and became public in 2017 June. In the present work, we simply re-ran the latest unWISE coaddition code (Meisner et al. 2017a) on inputs including this additional year of publicly available NEOWISER frames. The resulting set of full-depth coadds uniformly incorporates all publicly available W1 and W2 exposures, with observation dates ranging from 2010 January 7 to 2016 December 13. The inputs consisted of ? 10.5 million frames per band, totaling ? 140 terabytes of single-exposure pixel data.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/NEOWISER/Color
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      NEOWISER W2-W1
%Aladin.Tree        Image/Infrared/WISE/NEOWISER
%Aladin.HpxParam    8 image color equatorial png
%Aladin.Date        2018-03-05T05:57Z

%ActionName         P-NEOWISER-W1.hpx
%Description        NEOWISER W1
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/NEOWISER/W1
%VerboseDescr       The NEOWISE project is the asteroid-hunting portion of the Wide-field Infrared Survey Explorer (WISE) mission. Funded by NASA's Planetary Science Division, NEOWISE harvests measurements of asteroids and comets from the WISE images and provides a rich archive for searching WISE data for solar system objects. Here we update our full-depth coadds by folding in the most recently published year of W1/W2 exposures released by NEOWISER. These new single-frame data were acquired between 2015 December 13 and 2016 December 13, and became public in 2017 June. In the present work, we simply re-ran the latest unWISE coaddition code (Meisner et al. 2017a) on inputs including this additional year of publicly available NEOWISER frames. The resulting set of full-depth coadds uniformly incorporates all publicly available W1 and W2 exposures, with observation dates ranging from 2010 January 7 to 2016 December 13. The inputs consisted of ? 10.5 million frames per band, totaling ? 140 terabytes of single-exposure pixel data.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/NEOWISER/W1
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      NEOWISER W1 (3.4um)
%Aladin.Tree        Image/Infrared/WISE/NEOWISER
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2018-01-30T21:24Z

%ActionName         P-NEOWISER-W2.hpx
%Description        NEOWISER W2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/NEOWISER/W2
%VerboseDescr       The NEOWISE project is the asteroid-hunting portion of the Wide-field Infrared Survey Explorer (WISE) mission. Funded by NASA's Planetary Science Division, NEOWISE harvests measurements of asteroids and comets from the WISE images and provides a rich archive for searching WISE data for solar system objects. Here we update our full-depth coadds by folding in the most recently published year of W1/W2 exposures released by NEOWISER. These new single-frame data were acquired between 2015 December 13 and 2016 December 13, and became public in 2017 June. In the present work, we simply re-ran the latest unWISE coaddition code (Meisner et al. 2017a) on inputs including this additional year of publicly available NEOWISER frames. The resulting set of full-depth coadds uniformly incorporates all publicly available W1 and W2 exposures, with observation dates ranging from 2010 January 7 to 2016 December 13. The inputs consisted of â?¼ 10.5 million frames per band, totaling â?¼ 140 terabytes of single-exposure pixel data.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/NEOWISER/W2
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      NEOWISER W2 (4.6um)
%Aladin.Tree        Image/Infrared/WISE/NEOWISER
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2018-02-09T00:59Z

%ActionName         P-NVSS.hpx
%Description        NVSS - The NRAO VLA Sky Survey (intensity maps)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/NVSS/intensity
%VerboseDescr       The NRAO VLA Sky Survey (NVSS) is a 1.4 GHz continuum survey covering the entire sky north of -40 deg declination. NVSS intensity maps - resampled in Healpix by CDS
%Copyright          Copyright 2009 Associated Universities, Inc. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
%Origin             CDS
%Id                 P/NVSS
%Aladin.Profile     >6.1
%Copyright.Url      http://www.nrao.edu/archives/archpolicy.shtml
%SkyFraction        0.8242
%Aladin.XLabel      NVSS
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-05
%Aladin.HpxParam    5 image equatorial jpeg fits
%Aladin.Date        2015-04-07T13:09Z

%ActionName         P-Neptune-Voyager2.hpx
%Description        Neptune Voyager2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Neptune_Voyager2
%VerboseDescr       This map of Neptune was created from 9 sets images taken by the Voyager 2 spacecraft in August 1989 from a distance of approximately 10 million km. Each set consisted of images taken through orange, green and blue filters. These were used as red, green and blue, respectively. This means that a total of 27 images was used.
%Origin             CDS
%Id                 P/Neptune/Voyager2
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Neptune/Voyager2
%Aladin.Tree        Solar system/Neptune
%Aladin.HpxParam    3 image color neptune jpeg
%Aladin.Date        2018-01-23T13:30Z

%ActionName         P-Nobeyama-3cm.hpx
%Description        Nobeyama 10 GHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Nobeyama_3cm
%VerboseDescr       10 GHz (3cm) radio continuum survey of the Galactic plane made by the Nobeyama Radio Observatory using the 45-m telescope, at the resolution of 3?. Units: mJy/Beam.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/Nobeyama/3cm
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.005066
%Aladin.XLabel      Nobeyama 3cm
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-22T15:44Z

%ActionName         P-Oberon-Voyager.hpx
%Description        Oberon Voyager
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Oberon_Voyager
%VerboseDescr       Oberon Uranus satellite map mosaicked with Voyager imagery by USGS
%Copyright          Caltech/JPL/NASA
%Origin             CDS
%Id                 P/Oberon/Voyager
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Oberon/Voyager
%Aladin.Tree        Solar system/Uranus/Oberon
%Aladin.HpxParam    3 image color oberon jpeg
%Aladin.Date        2018-01-31T06:36Z

%ActionName         P-PARKES-150MHz.hpx
%Description        Parkes 150 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/PARKES_150MHz
%VerboseDescr       Equatorial plane survey at 150 MHz using the Parkes 64-m radio telescope, at a resolution of 2.2deg. Units:KTB \nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/PARKES/150MHz
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.4319
%Aladin.XLabel      PARKES 150MHz
%Aladin.Tree        Image/Radio/PARKES
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-09-01T13:29Z

%ActionName         P-PARKES-6cm.hpx
%Description        Parkes 6cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/PARKES_6cm
%VerboseDescr       Galactic plane survey at 5 GHz using the Parkes 64-m radio telescope, at a resolution of 4.1?. Units: mKTB. \nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/PARKES/6cm
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.01092
%Aladin.XLabel      PARKES 6cm
%Aladin.Tree        Image/Radio/PARKES
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-25T13:54Z

%ActionName         P-PARKES-85MHz.hpx
%Description        Parkes 85 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1474625760  2016/09/23 12:16:00
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/PARKES_85MHz
%VerboseDescr       Equatorial plane survey at 85 MHz using the Parkes 64-m radio telescope, at a resolution of 3.5deg. Units:KTB\nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/PARKES/85MHz
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.4319
%Aladin.XLabel      PARKES 85MHz
%Aladin.Tree        Image/Radio/PARKES
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-09-01T13:50Z

%ActionName         P-PLANCK-HFIColor.hpx.outreach
%Description        PLANCK HFI color composition 353-545-857 GHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/PLANCK/HFIColor353-545-857
%Copyright          from ESA
%Copyright.url      http://pla.esac.esa.int/pla
%Aladin.Profile     >6.1 undergraduate
%Aladin.XLabel      PLANCK-HFI color 353-545-857 GHz
%Aladin.HpxParam    3 gal color jpeg
%Aladin.MenuNumber  B3a

%ActionName         P-PLANCK-R2-CMB.hpx
%Description        PLANCK Maps of the CMB fluctuations.
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/COM_CMB_IQU-smica-field-Int_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/CMB
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 CMB
%Aladin.Tree        Image/Radio/PLANCK/R2
%Aladin.MenuNumber  05-04-03
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-06T13:52Z

%ActionName         P-PLANCK-R2-HFI-color.hpx
%Description        PLANCK R2 HFI color composition 353-545-857 GHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_Color_353_545_857
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI/color
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI color
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-02-00
%Aladin.HpxParam    3 image color galactic jpeg
%Aladin.Date        2015-02-06T13:38Z

%ActionName         P-PLANCK-R2-HFI100.hpx
%Description        PLANCK R2 nominal frequency HFI map 100Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_100_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI100
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI100
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-08
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:46Z

%ActionName         P-PLANCK-R2-HFI143.hpx
%Description        PLANCK R2 nominal frequency HFI map 143Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_143_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI143
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI143
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-07
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:49Z

%ActionName         P-PLANCK-R2-HFI217.hpx
%Description        PLANCK R2 nominal frequency HFI map 217Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_217_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI217
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI217
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-06
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:54Z

%ActionName         P-PLANCK-R2-HFI353.hpx
%Description        PLANCK R2 nominal frequency HFI map 353Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_353_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI353
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI353
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-05
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T17:37Z

%ActionName         P-PLANCK-R2-HFI545.hpx
%Description        PLANCK R2 nominal frequency HFI map 545Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_545_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI545
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI545
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-04
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T17:41Z

%ActionName         P-PLANCK-R2-HFI857.hpx
%Description        PLANCK R2 nominal frequency HFI map 857Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/HFI_SkyMap_857_2048_R2.00
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/HFI857
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 HFI857
%Aladin.Tree        Image/Radio/PLANCK/R2/HFI
%Aladin.MenuNumber  05-04-xR2-01-03
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T17:52Z

%ActionName         P-PLANCK-R2-LFI-color.hpx
%Description        PLANCK R2 LFI color composition 30-44-70 GHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/LFI_Color_30_44_70
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/LFI/color
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 LFI color
%Aladin.Tree        Image/Radio/PLANCK/R2/LFI
%Aladin.MenuNumber  05-04-xR2-02-00
%Aladin.HpxParam    3 image color galactic jpeg
%Aladin.Date        2015-02-06T12:09Z

%ActionName         P-PLANCK-R2-LFI030.hpx
%Description        PLANCK R2 nominal frequency LFI map 30 Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/LFI_SkyMap_030_1024_R2.01
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/LFI030
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 LFI030
%Aladin.Tree        Image/Radio/PLANCK/R2/LFI
%Aladin.MenuNumber  05-04-xR2-02-03
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:40Z

%ActionName         P-PLANCK-R2-LFI044.hpx
%Description        PLANCK R2 nominal frequency LFI map 44 Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/LFI_SkyMap_044_1024_R2.01
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/LFI044
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 LFI044
%Aladin.Tree        Image/Radio/PLANCK/R2/LFI
%Aladin.MenuNumber  05-04-xR2-02-02
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:42Z

%ActionName         P-PLANCK-R2-LFI070.hpx
%Description        PLANCK R2 nominal frequency LFI map 70Ghz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/PLANCK/R2/LFI_SkyMap_070_2048_R2.01
%VerboseDescr       The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
%Copyright          Planck Legacy Archive
%Origin             CDS
%Id                 P/PLANCK/R2/LFI070
%Aladin.Profile     >6.1
%Copyright.Url      http://pla.esac.esa.int/pla
%SkyFraction        1
%Aladin.XLabel      PLANCK R2 LFI070
%Aladin.Tree        Image/Radio/PLANCK/R2/LFI
%Aladin.MenuNumber  05-04-xR2-02-01
%Aladin.HpxParam    3 image galactic png fits
%Aladin.Date        2015-02-05T16:29Z

%ActionName         P-PanSTARRS-DR1-color-z-zg-g.hpx
%Description        PanSTARRS DR1 color (from bands z and g)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-PanSTARRS-DR1-color-z-zg-g_0.hpx availability=0
%SeeAction          P-PanSTARRS-DR1-color-z-zg-g_1.hpx availability=0
%SeeAction          P-PanSTARRS-DR1-color-z-zg-g_2.hpx availability=0
%VerboseDescr       Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3? Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5? point source limiting sensitivities in the stacked 3? Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (?ra, ?dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
%Copyright          PS1 Science Consortium
%Origin             CDS
%Id                 P/PanSTARRS/DR1/color-z-zg-g
%Aladin.Profile     >6.1
%Copyright.Url      http://panstarrs.stsci.edu/
%SkyFraction        0.7812
%Aladin.XLabel      PanSTARRS DR1 color (from bands z and g)
%Aladin.Tree        Image/Optical/PanSTARRS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    11 image color equatorial jpeg
%Aladin.Date        2017-04-20T12:51Z

%ActionName         P-PanSTARRS-DR1-g.hpx
%Description        PanSTARRS DR1 g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-PanSTARRS-DR1-g_0.hpx availability=0
%SeeAction          P-PanSTARRS-DR1-g_1.hpx availability=0
%SeeAction          P-PanSTARRS-DR1-g_2.hpx availability=0
%VerboseDescr       Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3? Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5? point source limiting sensitivities in the stacked 3? Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (?ra, ?dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
%Copyright          PS1 Science Consortium
%Origin             CDS
%Id                 P/PanSTARRS/DR1/g
%Aladin.Profile     >6.1
%Copyright.Url      http://panstarrs.stsci.edu/
%SkyFraction        0.7579
%Aladin.XLabel      PanSTARRS DR1 g
%Aladin.Tree        Image/Optical/PanSTARRS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    11 image equatorial jpeg fits
%Aladin.Date        2017-12-19T14:51Z

%ActionName         P-PanSTARRS-DR1-i.hpx
%Description        PanSTARRS DR1 i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/Pan-STARRS/DR1/i
%VerboseDescr       Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3? Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5? point source limiting sensitivities in the stacked 3? Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (?ra, ?dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
%Copyright          PS1 Science Consortium
%Origin             CDS
%Id                 P/PanSTARRS/DR1/i
%Aladin.Profile     >6.1
%Copyright.Url      http://panstarrs.stsci.edu/
%SkyFraction        0.7628
%Aladin.XLabel      PanSTARRS DR1 i
%Aladin.Tree        Image/Optical/PanSTARRS
%Aladin.HpxParam    11 image equatorial fits jpeg
%Aladin.Date        2019-07-01T13:05Z

%ActionName         P-PanSTARRS-DR1-y.hpx
%Description        PanSTARRS DR1 y
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Pan-STARRS/DR1/y
%VerboseDescr       Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3? Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5? point source limiting sensitivities in the stacked 3? Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (?ra, ?dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
%Copyright          PS1 Science Consortium
%Origin             CDS
%Id                 P/PanSTARRS/DR1/y
%Aladin.Profile     >6.1
%Copyright.Url      http://panstarrs.stsci.edu/
%SkyFraction        0.7582
%Aladin.XLabel      PanSTARRS DR1 y
%Aladin.Tree        Image/Optical/PanSTARRS
%Aladin.HpxParam    11 image equatorial fits jpeg
%Aladin.Date        2018-11-12T17:48Z

%ActionName         P-PanSTARRS-DR1-z.hpx
%Description        PanSTARRS DR1 z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-PanSTARRS-DR1-z_0.hpx availability=0
%SeeAction          P-PanSTARRS-DR1-z_1.hpx availability=1
%SeeAction          P-PanSTARRS-DR1-z_2.hpx availability=0
%VerboseDescr       Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3? Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5? point source limiting sensitivities in the stacked 3? Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (?ra, ?dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
%Copyright          PS1 Science Consortium
%Origin             CDS
%Id                 P/PanSTARRS/DR1/z
%Aladin.Profile     >6.1
%Copyright.Url      http://panstarrs.stsci.edu/
%SkyFraction        0.7578
%Aladin.XLabel      PanSTARRS DR1 z
%Aladin.Tree        Image/Optical/PanSTARRS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    11 image equatorial fits jpeg
%Aladin.Date        2018-02-09T08:38Z

%ActionName         P-Pluto-NewHorizons-Jul2017-300m.hpx
%Description        Pluto NewHorizons-Jul2017-300m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Pluto_NewHorizons-Jul2017-300m
%VerboseDescr       This detailed, high-quality global mosaic of Pluto was assembled from nearly all of the highest-resolution images obtained by the Long-Range Reconnaissance Imager (LORRI) and the Multispectral Visible Imaging Camera (MVIC) on New Horizons. The mosaic is the most detailed and comprehensive global view yet of Pluto?s surface using New Horizons data. It includes topography data of the hemisphere visible to New Horizons during the spacecraft?s closest approach. The topography is derived from digital stereo-image mapping tools that measure the parallax ? or the difference in the apparent relative positions ? of features on the surface obtained at different viewing angles during the encounter. Scientists use these parallax displacements of high and low terrain to estimate landform heights.
%Copyright          Planetary Data System, from USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Pluto/NewHorizons-Jul2017-300m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Pluto/NewHorizons-Jul2017-300m
%Aladin.Tree        Solar system/Pluto
%Aladin.HpxParam    3 image color pluto jpeg
%Aladin.Date        2018-01-21T10:45Z

%ActionName         P-RASS-HardBand.hpx
%Description        ROSAT All Sky Survey (RASS) - 0.5-2.4 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1461076880  2016/04/19 16:41:20
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/RASS_IM2
%VerboseDescr       Allsky survey in the Hard energy band (0.5-2.4 keV). The map in counts/sec should be multiplied by 5.24559 to get counts per HEALPix pixel. Angular resolution of 1.8'. Units: Counts/sec\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/RASS/HardBand
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      RASS 0.5-2.4 keV
%Aladin.Tree        Image/X/RASS
%Aladin.MenuNumber  01-02a
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-12-16T16:49Z

%ActionName         P-RASS-SoftBand.hpx
%Description        ROSAT All Sky Survey (RASS) - 0.1-0.4 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1461076880  2016/04/19 16:41:20
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/RASS_IM3
%VerboseDescr       Allsky survey in the Soft energy band (0.1-0.4 keV). The map in counts/sec should be multiplied by 5.24559 to get counts per HEALPix pixel. Angular resolution of 1.8'. Units: Counts/sec\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/RASS/SoftBand
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      RASS  0.1-0.4 keV
%Aladin.Tree        Image/X/RASS
%Aladin.MenuNumber  01-02a
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-12-16T16:54Z

%ActionName         P-RASS.hpx
%Description        ROSAT All Sky Survey (RASS) - 0.1-2.4 keV
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1461076880  2016/04/19 16:41:20
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/RASS
%VerboseDescr       Allsky survey in the total energy band (0.1-2.4 keV). The map in counts/sec should be multiplied by 5.24559 to get counts per HEALPix pixel. Angular resolution of 1.8'. Units: Counts/sec\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/RASS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      RASS 0.1-2.4 keV
%Aladin.Tree        Image/X/RASS
%Aladin.MenuNumber  01-02a
%Aladin.HpxParam    3 image galactic jpeg fits
%Aladin.Date        2013-06-24T15:02Z

%ActionName         P-ROSATWFC-F1.hpx
%Description        ROSAT Wide Field Camera F1 (15-27 PHz)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ROSATWFC-new/ROSAT-WFC1
%VerboseDescr       During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
%Copyright          University of Leicester used by permission (no restrictions on not for profit use)
%Origin             CDS
%Id                 P/ROSATWFC/F1
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        0.9714
%Aladin.XLabel      ROSAT WFC F1 (15-27 PHz)
%Aladin.Tree        Image/UV/ROSATWFC
%Aladin.MenuNumber  02-xx
%Aladin.HpxParam    3 image equatorial png fits
%Aladin.Date        2016-02-09T15:40Z

%ActionName         P-ROSATWFC-F2.hpx
%Description        ROSAT Wide Field Camera F2 (21-50 PHz)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ROSATWFC-new/ROSAT-WFC2
%VerboseDescr       obs_description      = During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
%Copyright          University of Leicester used by permission (no restrictions on not for profit use)
%Origin             CDS
%Id                 P/ROSATWFC/F2
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        0.9714
%Aladin.XLabel      ROSAT-WFC-F2 (21-50 PHz)
%Aladin.Tree        Image/UV/ROSATWFC
%Aladin.MenuNumber  02-xx
%Aladin.HpxParam    3 image equatorial png fits
%Aladin.Date        2016-02-09T15:19Z

%ActionName         P-ROSATWFC-color.hpx
%Description        ROSAT Wide Field Camera Color composition
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/ROSATWFC-new/ROSAT-WFC-color
%VerboseDescr       During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
%Copyright          University of Leicester used by permission (no restrictions on not for profit use)
%Origin             CDS
%Id                 P/ROSATWFC/color
%Aladin.Profile     >6.1
%Copyright.Url      http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
%SkyFraction        0.9714
%Aladin.XLabel      ROSAT color
%Aladin.Tree        Image/UV/ROSATWFC
%Aladin.MenuNumber  02-xx
%Aladin.HpxParam    3 image color equatorial png
%Aladin.Date        2016-01-28T16:13Z

%ActionName         P-Rhea-Cassini-PIA12803.hpx
%Description        Rhea Cassini PIA12803
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Rhea_Cassini-PIA12803
%VerboseDescr       This global digital map of Saturn's moon Rhea was created using data obtained by NASA's Cassini and Voyager spacecraft. The map is an equidistant projection and has a scale of 417 meters (1,400 feet) per pixel in the full size version. The mean radius of Rhea used for projection of this map is 764.1 kilometers (474.8 miles). Six Voyager images fill gaps in Cassini's coverage of the north pole. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate in Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.
%Copyright          JPL/PhotoJournal
%Origin             CDS
%Id                 P/Rhea/Cassini-PIA12803
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Rhea/Cassini-PIA12803
%Aladin.Tree        Solar system/Saturn/Rhea
%Aladin.HpxParam    3 image color rhea jpeg
%Aladin.Date        2018-01-24T13:57Z

%ActionName         P-SCUBA-450em.hpx
%Description        SCUBA 450um emission maps
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SCUBA/Scuba450ALLSKY
%VerboseDescr       SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
%Copyright          SCUBA Legacy
%Origin             CDS
%Id                 P/SCUBA/450em
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy
%SkyFraction        0.003081
%Aladin.XLabel      SCUBA 450em
%Aladin.Tree        Image/Radio/SCUBA
%Aladin.MenuNumber  05-01-03
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2012-10-11T11:10Z

%ActionName         P-SCUBA-850em.hpx
%Description        SCUBA 850um emission maps
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SCUBA/Scuba850ALLSKY
%VerboseDescr       SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
%Copyright          SCUBA Legacy
%Origin             CDS
%Id                 P/SCUBA/850em
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy/
%SkyFraction        0.003577
%Aladin.XLabel      SCUBA 850em
%Aladin.Tree        Image/Radio/SCUBA
%Aladin.MenuNumber  05-01-04
%Aladin.HpxParam    7 image equatorial jpeg fits
%Aladin.Date        2012-10-11T07:15Z

%ActionName         P-SCUBA-850emi.hpx
%Description        SCUBA 850um emission maps - extended dataset
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SCUBA/Scuba850eALLSKY
%VerboseDescr       SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
%Copyright          SCUBA Legacy
%Origin             CDS
%Id                 P/SCUBA/850emi
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy/
%SkyFraction        0.003953
%Aladin.XLabel      SCUBA 850emi
%Aladin.Tree        Image/Radio/SCUBA
%Aladin.MenuNumber  05-01-05
%Aladin.HpxParam    7 image equatorial jpeg fits
%Aladin.Date        2012-10-10T10:33Z

%ActionName         P-SCUBA2-450em.hpx
%Description        SCUBA2 450um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SCUBA2/Scuba2_450
%VerboseDescr       The SCUBA2-450em Hierarchical Progressive Survey (HiPS) has been built from JCMT data via CADC archive and distributed by CDS.It sets together all SCUBA2 observations done in 450 filter between the beginning of the mission to the 1st of November 2014. SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope.
%Copyright          2014-2017 East Asian Observatory all rights reserved
%Origin             CDS
%Id                 P/SCUBA2/450em
%Aladin.Profile     >6.1
%Copyright.Url      http://www.eaobservatory.org/jcmt/contact/
%SkyFraction        0.01752
%Aladin.XLabel      SCUBA2 450em
%Aladin.Tree        Image/Radio/SCUBA
%Aladin.MenuNumber  05-01-01
%Aladin.HpxParam    9 image equatorial png jpeg fits
%Aladin.Date        2014-11-20T11:18Z

%ActionName         P-SCUBA2-850em.hpx
%Description        SCUBA2 850um
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SCUBA2/Scuba2_850
%VerboseDescr       The SCUBA2-450em Hierarchical Progressive Survey (HiPS) has been built from JCMT data via CADC archive and distributed by CDS.It sets together all SCUBA2 observations done in 450 filter between the beginning of the mission to the 1st of November 2014. SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope.
%Copyright          2014-2017 East Asian Observatory all rights reserved
%Origin             CDS
%Id                 P/SCUBA2/850em
%Aladin.Profile     >6.1
%Copyright.Url      http://www.eaobservatory.org/jcmt/contact/
%SkyFraction        0.01804
%Aladin.XLabel      SCUBA2 850em
%Aladin.Tree        Image/Radio/SCUBA
%Aladin.MenuNumber  05-01-02
%Aladin.HpxParam    9 image equatorial png jpeg fits
%Aladin.Date        2014-11-20T14:19Z

%ActionName         P-SDSS9-color-alt.hpx
%Description        SDSS9 color (g, r, i CDS color composition)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/color-alt
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data collection began in 2000, and the final imaging data release covers over 35% of the sky. This color composition is an CDS alternative to the orignal SLOAN color composition using the g, r an i original DR9 bands with a log transfer function and specifical cuts for each band.
%Copyright          Sloan Digital Sky Survey
%Origin             CDS
%Id                 P/SDSS9/color-alt
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/collaboration/#image-use
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 color-alt
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-00
%Aladin.HpxParam    10 image color equatorial png
%Aladin.Date        2016-05-29T00:46Z

%ActionName         P-SDSS9-color.hpx
%Description        SDSS9 color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-SDSS9-color_0.hpx availability=0
%SeeAction          P-SDSS9-color_1.hpx availability=10
%SeeAction          P-SDSS9-color_2.hpx availability=0
%SeeAction          P-SDSS9-color_3.hpx availability=0
%SeeAction          P-SDSS9-color_4.hpx availability=9999
%SeeAction          P-SDSS9-color_5.hpx availability=11
%SeeAction          P-SDSS9-color_6.hpx availability=1055
%SeeAction          P-SDSS9-color_7.hpx availability=14
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data collection began in 2000, and the final imaging data release covers over 35% of the sky. This color composition is an CDS alternative to the orignal SLOAN color composition using the g, r an i original DR9 bands with a log transfer function and specifical cuts for each band.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS
%Origin             CDS
%Id                 P/SDSS9/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 color
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-01 lite
%Aladin.HpxParam    10 image color equatorial jpeg
%Aladin.Date        2014-10-24T15:12Z

%ActionName         P-SDSS9-g.hpx
%Description        SDSS9 band g
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/band-g
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS	Sloan Digital Sky Survey
%Origin             CDS
%Id                 P/SDSS9/g
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/	http://www.sdss.org/collaboration/#image-use
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 g
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-03
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2016-01-20T13:49Z

%ActionName         P-SDSS9-i.hpx
%Description        SDSS9 band i
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/band-i
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS
%Origin             CDS
%Id                 P/SDSS9/i
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 i
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-05
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2014-12-17T22:14Z

%ActionName         P-SDSS9-r.hpx
%Description        SDSS9 band r
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/band-r
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS
%Origin             CDS
%Id                 P/SDSS9/r
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 r
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-04
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2014-10-24T15:24Z

%ActionName         P-SDSS9-u.hpx
%Description        SDSS9 band u
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/band-u
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS
%Origin             CDS
%Id                 P/SDSS9/u
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 u
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-02
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2015-02-11T20:58Z

%ActionName         P-SDSS9-z.hpx
%Description        SDSS9 band z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SDSS/DR9/band-z
%VerboseDescr       The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
%Copyright          SLOAN Digitized Sky Survey - Healpixed by CDS
%Origin             CDS
%Id                 P/SDSS9/z
%Aladin.Profile     >6.1
%Copyright.Url      http://www.sdss.org/
%SkyFraction        0.3562
%Aladin.XLabel      SDSS9 z
%Aladin.Tree        Image/Optical/SDSS
%Aladin.MenuNumber  03-02-06
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2015-03-18T01:39Z

%ActionName         P-SGPS-CONT.hpx
%Description        21-cm continuum - Southern Galactic Plane Survey (SGPS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SGPS_CONT
%VerboseDescr       Radio continuum emission of the atomic hydrogen line, using the Australia Telescope Compact Array and Parkes Radiotelescopes, at a resolution of 2.2?. Units: Jy/beam\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SGPS/CONT
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.006203
%Aladin.XLabel      SGPS CONT- Southern Galactic Plane Survey
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-08
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2015-02-25T12:02Z

%ActionName         P-SGPS-II.hpx
%Description        Southern Galactic Plane Survey (SGPS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SGPS_II
%VerboseDescr       Atomic Hydrogen (integrated intensity map - continuum removed) emission using the Australia Telescope Compact Array and Parkes Radiotelescopes, at a resolution of 2.2? (SGPS I) to 3.3? (SGPS II). Units: K m/s\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SGPS/II
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.009468
%Aladin.XLabel      SGPS - Southern Galactic Plane Survey
%Aladin.Tree        Image/Gas-lines/HI
%Aladin.MenuNumber  06-08
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2015-02-25T11:52Z

%ActionName         P-SHASSA-CONT.hpx
%Description        SHASSA Continuum
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SHASSA_CONT
%VerboseDescr       Continuum emission from the Southern H-Alpha Sky Survey Atlas (SHASSA) (declinations less than +15 degrees). Units are dR. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SHASSA/CONT
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.6428
%Aladin.XLabel      SHASSA Continuum
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2018-12-05T13:19Z

%ActionName         P-SHASSA-DU.hpx
%Description        SHASSA DU - Continuum
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SHASSA-DU
%VerboseDescr       The Southern H-Alpha Sky Survey Atlas is the product of a wide-angle digital imaging survey of the H-alpha emission from the warm ionized interstellar gas of our Galaxy. This atlas covers the southern hemisphere sky (declinations less than +15 degrees). The observations were taken with a robotic camera operating at Cerro Tololo Inter-American Observatory (CTIO) in Chile.
%Copyright          By courtesy of Swarthmore College Incorporated
%Origin             CDS
%Id                 P/SHASSA/DU
%Aladin.Profile     >6.1
%Copyright.Url      http://amundsen.astro.swarthmore.edu/SHASSA/ack.html
%SkyFraction        0.6618
%Aladin.XLabel      SHASSA DU
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.MenuNumber  06-02-02
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-04-22T16:27Z

%ActionName         P-SHASSA-FL.hpx
%Description        SHASSA FL - Continuum subtract.
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SHASSA-FL
%VerboseDescr       The Southern H-Alpha Sky Survey Atlas is the product of a wide-angle digital imaging survey of the H-alpha emission from the warm ionized interstellar gas of our Galaxy. This atlas covers the southern hemisphere sky (declinations less than +15 degrees). The observations were taken with a robotic camera operating at Cerro Tololo Inter-American Observatory (CTIO) in Chile.
%Copyright          By courtesy of Swarthmore College Incorporated
%Origin             CDS
%Id                 P/SHASSA/FL
%Aladin.Profile     >6.1
%Copyright.Url      http://amundsen.astro.swarthmore.edu/SHASSA/ack.html
%SkyFraction        0.6615
%Aladin.XLabel      SHASSA FL
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.MenuNumber  06-02-03
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-04-22T16:17Z

%ActionName         P-SHASSA-H.hpx
%Description        SHASSA H - H-alpha emission
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SHASSA-H3
%VerboseDescr       The Southern H-Alpha Sky Survey Atlas is the product of a wide-angle digital imaging survey of the H-alpha emission from the warm ionized interstellar gas of our Galaxy. This atlas covers the southern hemisphere sky (declinations less than +15 degrees). The observations were taken with a robotic camera operating at Cerro Tololo Inter-American Observatory (CTIO) in Chile.
%Copyright          By courtesy of Swarthmore College Incorporated
%Origin             CDS
%Id                 P/SHASSA/H
%Aladin.Profile     >6.1
%Copyright.Url      http://amundsen.astro.swarthmore.edu/SHASSA/index.html	http://amundsen.astro.swarthmore.edu/SHASSA/ack.html
%SkyFraction        0.6615
%Aladin.XLabel      SHASSA H
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.MenuNumber  06-02-01
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2014-04-22T12:06Z

%ActionName         P-SHASSA-HA.hpx
%Description        SHASSA H-alpha
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SHASSA_HA
%VerboseDescr       Southern H-Alpha Sky Survey Atlas (SHASSA) (declinations less than +15 degrees). This map has been generated with the Ha images. Units are dR and the angular resolution is approximately 1 arcminute. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SHASSA/HA
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.6428
%Aladin.XLabel      SHASSA H-alpha
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2018-12-04T12:38Z

%ActionName         P-SHASSA-SM.hpx
%Description        SHASSA SM
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SHASSA_SM
%VerboseDescr       Southern H-Alpha Sky Survey Atlas (SHASSA) (declinations less than +15 degrees). This map has been generated with the Smoothed data (median filtered to 5 pixels, or 4.0 arcminute resolution to remove star residuals better). Units are dR. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SHASSA/SM
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.6438
%Aladin.XLabel      SHASSA SM - Smoothed Continuum subtracted
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2018-12-04T12:46Z

%ActionName         P-SHASSA.hpx
%Description        SHASSA Continuum Subtracted
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SHASSA
%VerboseDescr       Southern H-Alpha Sky Survey Atlas (SHASSA) (declinations less than +15 degrees). This map is continuum-corrected (the difference of the H-Alpha and Continuum images). Units are dR. Healpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SHASSA
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.6428
%Aladin.XLabel      SHASSA Continuum Subtracted
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2018-12-06T10:03Z

%ActionName         P-SHS.hpx
%Description        SHS - digitized H-alpha photographic survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/SHS
%VerboseDescr       The UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory completed a narrow-band H? plus [Nii] 6548, 6584A-survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide-field photographic survey and the only one undertaken in a narrow-band, is now an online digital data product of the Wide-Field Astronomy Unit of the Royal Observatory Edinburgh (ROE). The original survey films were scanned by the SuperCOSMOS measuring machine at the Royal Observatory, Edinburgh, to provide the online digital atlas called the SuperCOSMOS H? Survey (SHS). The SuperCOSMOS Halpha Survey - digitized H-alpha photographic survey of the Southern Galactic Plane, taken by the AAO/UKST was resampled in Healpix by CDS.
%Copyright          By courtesy of WFAU, AAO/UKST, PPARC/STFC
%Origin             CDS
%Id                 P/SHS
%Aladin.Profile     >6.1
%Copyright.Url      http://www-wfau.roe.ac.uk/sss/halpha/
%SkyFraction        0.09776
%Aladin.XLabel      SHS
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.MenuNumber  06-01a
%Aladin.HpxParam    10 image equatorial png jpeg fits
%Aladin.Date        2014-04-22T16:35Z

%ActionName         P-SIM.hpx
%Description        SIM
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                http://alasky.u-strasbg.fr/ancillary/simbad-biblio/cubes/1990-now
%Origin             CDS
%Id                 P/SIM
%Aladin.Profile     >6.1
%SkyFraction        1
%Aladin.XLabel      P/SIM
%Aladin.Tree        Cube
%Aladin.HpxParam    0 cube equatorial png fits
%Aladin.Date        2019-03-25T11:29Z

%ActionName         P-SPITZER-IRAC1.hpx
%Description        IRAC1  survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/IRAC1
%VerboseDescr       Composite map from Spitzer Legacy Programs GLIMPSE: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (Churchwell E. + Benjamin R.) C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/IRAC1
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01449
%Aladin.XLabel      SPITZER IRAC1
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-01
%Aladin.HpxParam    9 image galactic jpeg fits
%Aladin.Date        2011-07-07T11:40Z

%ActionName         P-SPITZER-IRAC2.hpx
%Description        IRAC2  survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/IRAC2
%VerboseDescr       Composite map from Spitzer Legacy Programs GLIMPSE: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (Churchwell E. + Benjamin R.) C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/IRAC2
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01448
%Aladin.XLabel      SPITZER IRAC2
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-02
%Aladin.HpxParam    9 image galactic jpeg fits
%Aladin.Date        2011-07-06T15:52Z

%ActionName         P-SPITZER-IRAC3.hpx
%Description        IRAC3  survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/IRAC3
%VerboseDescr       Composite map from Spitzer Legacy Programs GLIMPSE: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (Churchwell E. + Benjamin R.) C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/IRAC3
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01447
%Aladin.XLabel      SPITZER IRAC3
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-03
%Aladin.HpxParam    9 image galactic jpeg fits
%Aladin.Date        2011-07-06T13:38Z

%ActionName         P-SPITZER-IRAC4.hpx
%Description        IRAC4  survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/IRAC4
%VerboseDescr       Composite map from Spitzer Legacy Programs GLIMPSE: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (Churchwell E. + Benjamin R.) C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/IRAC4
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01448
%Aladin.XLabel      SPITZER IRAC4
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-04
%Aladin.HpxParam    9 image galactic jpeg fits
%Aladin.Date        2011-07-06T08:46Z

%ActionName         P-SPITZER-MIPS1.hpx
%Description        MIPS1  survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/MIPS1
%VerboseDescr       Composite map from Spitzer Legacy Programs MIPSGAL: A 24 and 70 Micron Survey of the Inner Galactic Disk with MIPS (Carey S.) C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/MIPS1
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01872
%Aladin.XLabel      SPITZER MIPS1
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-05
%Aladin.HpxParam    8 image galactic jpeg fits
%Aladin.Date        2017-03-27T11:44Z

%ActionName         P-SPITZER-MIPS2.hpx
%Description        MIPS2 survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/MIPS2
%VerboseDescr       Composite map from Spitzer Legacy Programs C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/MIPS2
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.006882
%Aladin.XLabel      SPITZER MIPS2
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-06
%Aladin.HpxParam    7 image equatorial jpeg fits
%Aladin.Date        2017-03-27T14:12Z

%ActionName         P-SPITZER-MIPS3.hpx
%Description        MIPS3 survey in Healpix
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/MIPS3
%VerboseDescr       Composite map from Spitzer Legacy Programs C2D: From Molecular Cores to Planet-Forming Disks (Evans N.) Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds (Padgett D.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/MIPS3
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.006329
%Aladin.XLabel      SPITZER MIPS3
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-07
%Aladin.HpxParam    6 image equatorial jpeg fits
%Aladin.Date        2017-03-27T14:25Z

%ActionName         P-SPITZER-color.hpx
%Description        IRAC HEALPix survey, color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-SPITZER-color_0.hpx availability=9999
%SeeAction          P-SPITZER-color_1.hpx availability=9999
%SeeAction          P-SPITZER-color_2.hpx availability=9999
%SeeAction          P-SPITZER-color_3.hpx availability=1055
%VerboseDescr       Composite color map from Spitzer Legacy Programs GLIMPSE: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (Churchwell E. + Benjamin R.) SAGE: Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (Meixner M.) SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally- Disrupted, Low-Metallicity Small Magellanic Cloud (Gordon K.) SINGS: The Spitzer Infrared Nearby Galaxies Survey - Physics of the Star-Forming ISM and Galaxy Evolution (Kennicutt R.)
%Copyright          Spitzer mission - JPL/NASA
%Origin             CDS
%Id                 P/SPITZER/color
%Aladin.Profile     >6.1
%Copyright.Url      https://www.jpl.nasa.gov/copyrights.php
%SkyFraction        0.01215
%Aladin.XLabel      SPITZER color
%Aladin.Tree        Image/Infrared/Spitzer
%Aladin.MenuNumber  04-03-00 lite
%Aladin.HpxParam    9 image color galactic jpeg
%Aladin.Date        2011-07-09T09:45Z

%ActionName         P-STOCKERT+VILLAELISA-1420MHz.hpx
%Description        Stockert + Villa Elisa 1420 MHz
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/STOCKERT+VILLAELISA_1420MHz
%VerboseDescr       All-sky survey at 1420 MHz using the combination of the 25-mStockert and 30-m Villa Elisa telescopes, at a resolution of 36?. Units: mKTB. \nHealpix map built by D. Paradis (IRAP/CADE).
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/STOCKERT+VILLAELISA/1420MHz
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      STOCKERT+VILLAELISA 1420MHz
%Aladin.Tree        Image/Radio/STOCKERT
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-29T12:58Z

%ActionName         P-STOCKERT-11cm.hpx
%Description        Stockert 11cm
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/STOCKERT_11cm
%VerboseDescr       Northern Galactic plane survey at 2720 MHz using the Stockert 25-m telescope, at a resolution of 21?. Units: mKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/STOCKERT/11cm
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.1
%Aladin.XLabel      STOCKERT 11cm
%Aladin.Tree        Image/Radio/STOCKERT
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2016-08-23T11:00Z

%ActionName         P-SUMSS.hpx
%Description        The Survey University Molonglo Sky Survey (SUMSS)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/SUMSS
%VerboseDescr       The survey of the radio sky at 843 MHz covers the whole sky south of declination -30 degrees with abs(b)>10 degrees. The Galactic Plane region abs(b)<10 degrees is covered by the second epoch Molonglo Galactic Plane Survey. Resolution: 45??. Units: Jy/beam\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/SUMSS
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.2544
%Aladin.XLabel      SUMSS - 843 MHz
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-xx
%Aladin.HpxParam    4 image galactic png jpeg fits
%Aladin.Date        2015-02-02T11:18Z

%ActionName         P-SUZAKU.hpx
%Description        Suzaku public data image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1488873956  2017/03/07 10:05:56
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/suzaku/
%VerboseDescr       Superposition of Suzaku pseudo-color images, no exposure correction.
%Copyright          DARTS at JAXA/ISAS
%Origin             JAXA
%Id                 P/SUZAKU
%Aladin.Profile     >6.1
%Copyright.Url      http://darts.isas.jaxa.jp/astro/suzaku
%SkyFraction        1
%Aladin.XLabel      SUZAKU
%Aladin.Tree        Image/X
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2016/11/04 15:49:40

%ActionName         P-SWIFT_BAT_FLUX.hpx
%Description        Swift-BAT 70-month all-sray hard X-ray survey image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-SWIFT_BAT_FLUX_0.hpx availability=260
%SeeAction          P-SWIFT_BAT_FLUX_1.hpx availability=0
%SeeAction          P-SWIFT_BAT_FLUX_2.hpx availability=9999
%SeeAction          P-SWIFT_BAT_FLUX_3.hpx availability=9999
%VerboseDescr       Swift-BAT seudo-color images from 2004 December to 2010 September
%Copyright          Swift data archive
%Origin             JAXA
%Id                 P/SWIFT_BAT_FLUX
%Aladin.Profile     >6.1
%Copyright.Url      http://swift.gsfc.nasa.gov/sdc/swift_acknowledge.html
%SkyFraction        1
%Aladin.XLabel      SWIFT_BAT_FLUX
%Aladin.Tree        Image/X
%Aladin.MenuNumber  lite
%Aladin.HpxParam    6 image color equatorial png
%Aladin.Date        2016-10-25T07:17Z

%ActionName         P-Sun-euvi-aia304-2012.hpx
%Description        Sun euvi-aia304-2012
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Sun_euvi-aia304-2012
%VerboseDescr       this map has been extracted from a movie showing the evolution of the Sun's entire surface as seen in extreme ultraviolet light (304 angstroms) for the time period Jan 1 - Sep 27, 2012.
%Copyright          GSFC/NASA
%Origin             CDS
%Id                 P/Sun/euvi-aia304-2012
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Sun/euvi-aia304-2012
%Aladin.Tree        Solar system/Sun
%Aladin.HpxParam    3 image color sun-carrington jpeg
%Aladin.Date        2018-01-23T14:29Z

%ActionName         P-Swift-UVOT-cnt_B.hpx
%Description        Combined Swift UVOT counts: band B
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/B
%VerboseDescr       Summed counts for the Swift UVOT B band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_B
%Aladin.Profile     >6.1
%SkyFraction        0.01805
%Aladin.XLabel      Swift_UVOT_cnt_B
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-08T22:59Z

%ActionName         P-Swift-UVOT-cnt_U.hpx
%Description        Combined Swift UVOT counts: band U
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/U
%VerboseDescr       Summed counts for the Swift UVOT U band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_U
%Aladin.Profile     >6.1
%SkyFraction        0.0451
%Aladin.XLabel      Swift_UVOT_cnt_U
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-20T03:07Z

%ActionName         P-Swift-UVOT-cnt_UVM2.hpx
%Description        Combined Swift UVOT counts: band UVM2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/UVM2
%VerboseDescr       Summed counts for the Swift UVOT UVM2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_UVM2
%Aladin.Profile     >6.1
%SkyFraction        0.04769
%Aladin.XLabel      Swift_UVOT_cnt_UVM2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-31T16:05Z

%ActionName         P-Swift-UVOT-cnt_UVW1.hpx
%Description        Combined Swift UVOT counts: band UVW1
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/UVW1
%VerboseDescr       Summed counts for the Swift UVOT UVW1 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_UVW1
%Aladin.Profile     >6.1
%SkyFraction        0.0413
%Aladin.XLabel      Swift_UVOT_cnt_UVW1
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-22T01:43Z

%ActionName         P-Swift-UVOT-cnt_UVW2.hpx
%Description        Combined Swift UVOT counts: band UVW2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/UVW2
%VerboseDescr       Summed counts for the Swift UVOT UVW2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_UVW2
%Aladin.Profile     >6.1
%SkyFraction        0.04165
%Aladin.XLabel      Swift_UVOT_cnt_UVW2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-30T19:55Z

%ActionName         P-Swift-UVOT-cnt_V.hpx
%Description        Combined Swift UVOT counts: band V
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/V
%VerboseDescr       Summed counts for the Swift UVOT V band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_V
%Aladin.Profile     >6.1
%SkyFraction        0.02029
%Aladin.XLabel      Swift_UVOT_cnt_V
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-15T17:39Z

%ActionName         P-Swift-UVOT-cnt_WHITE.hpx
%Description        Combined Swift UVOT counts: band WHITE
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/cnt/WHITE
%VerboseDescr       Summed counts for the Swift UVOT WHITE band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/cnt_WHITE
%Aladin.Profile     >6.1
%SkyFraction        0.002868
%Aladin.XLabel      Swift_UVOT_cnt_WHITE
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-14T16:44Z

%ActionName         P-Swift-UVOT-exp_B.hpx
%Description        Combined Swift UVOT exposure: band B
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/B
%VerboseDescr       Summed exposure for the Swift UVOT B band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_B
%Aladin.Profile     >6.1
%SkyFraction        0.01805
%Aladin.XLabel      Swift_UVOT_exp_B
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-08T13:27Z

%ActionName         P-Swift-UVOT-exp_U.hpx
%Description        Combined Swift UVOT exposure: band U
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/U
%VerboseDescr       Summed exposure for the Swift UVOT U band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_U
%Aladin.Profile     >6.1
%SkyFraction        0.0451
%Aladin.XLabel      Swift_UVOT_exp_U
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-21T03:14Z

%ActionName         P-Swift-UVOT-exp_UVM2.hpx
%Description        Combined Swift UVOT exposure: band UVM2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/UVM2
%VerboseDescr       Summed exposure for the Swift UVOT UVM2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_UVM2
%Aladin.Profile     >6.1
%SkyFraction        0.04769
%Aladin.XLabel      Swift_UVOT_exp_UVM2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-04T19:16Z

%ActionName         P-Swift-UVOT-exp_UVW1.hpx
%Description        Combined Swift UVOT exposure: band UVW1
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/UVW1
%VerboseDescr       Summed exposure for the Swift UVOT UVW1 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_UVW1
%Aladin.Profile     >6.1
%SkyFraction        0.04367
%Aladin.XLabel      Swift_UVOT_exp_UVW1
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-24T01:47Z

%ActionName         P-Swift-UVOT-exp_UVW2.hpx
%Description        Combined Swift UVOT exposure: band UVW2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/UVW2
%VerboseDescr       Summed exposure for the Swift UVOT UVW2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_UVW2
%Aladin.Profile     >6.1
%SkyFraction        0.04165
%Aladin.XLabel      Swift_UVOT_exp_UVW2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-10-06T07:14Z

%ActionName         P-Swift-UVOT-exp_V.hpx
%Description        Combined Swift UVOT exposure: band V
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/V
%VerboseDescr       Summed exposure for the Swift UVOT V band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_V
%Aladin.Profile     >6.1
%SkyFraction        0.02029
%Aladin.XLabel      Swift_UVOT_exp_V
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-08T09:45Z

%ActionName         P-Swift-UVOT-exp_WHITE.hpx
%Description        Combined Swift UVOT exposure: band WHITE
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/exp/WHITE
%VerboseDescr       Summed exposure for the Swift UVOT WHITE band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/exp_WHITE
%Aladin.Profile     >6.1
%SkyFraction        0.002868
%Aladin.XLabel      Swift_UVOT_exp_WHITE
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-08-09T17:36Z

%ActionName         P-Swift-UVOT-int_B.hpx
%Description        Combined Swift UVOT intensities: band B
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/B
%VerboseDescr       Intensity map for the Swift UVOT B band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_B
%Aladin.Profile     >6.1
%SkyFraction        0.01805
%Aladin.XLabel      Swift_UVOT_int_B
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-08T22:59Z

%ActionName         P-Swift-UVOT-int_UVM2.hpx
%Description        Combined Swift UVOT intensities: band UVM2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/UVM2
%VerboseDescr       Intensity map for the Swift UVOT UVM2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_UVM2
%Aladin.Profile     >6.1
%SkyFraction        0.04769
%Aladin.XLabel      Swift_UVOT_int_UVM2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-01TZ00:00:00Z

%ActionName         P-Swift-UVOT-int_UVW1.hpx
%Description        Combined Swift UVOT intensities: band UVW1
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/UVW1
%VerboseDescr       Intensity map for the Swift UVOT UVW1 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_UVW1
%Aladin.Profile     >6.1
%SkyFraction        0.0413
%Aladin.XLabel      Swift_UVOT_int_UVW1
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-22T01:43Z

%ActionName         P-Swift-UVOT-int_UVW2.hpx
%Description        Combined Swift UVOT intensities: band UVW2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/UVW2
%VerboseDescr       Intensity map for the Swift UVOT UVW2 band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_UVW2
%Aladin.Profile     >6.1
%SkyFraction        0.04165
%Aladin.XLabel      Swift_UVOT_int_UVW2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-30T19:55Z

%ActionName         P-Swift-UVOT-int_U_UVW1_UVW2.hpx
%Description        Combined Swift UVOT intensities: color bands U-UVW1-UVW2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/color2
%VerboseDescr       Intensity map for the Swift UVOT U,UVW1,UVW2 bands for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_U_UVW1_UVW2
%Aladin.Profile     >6.1
%SkyFraction        0.0343
%Aladin.XLabel      Swift_UVOT_int_U_UVW1_UVW2
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial jpg
%Aladin.Date        2017-09-08T22:59Z

%ActionName         P-Swift-UVOT-int_V.hpx
%Description        Combined Swift UVOT intensities: band V
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/V
%VerboseDescr       Intensity map for the Swift UVOT V band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_V
%Aladin.Profile     >6.1
%SkyFraction        0.02029
%Aladin.XLabel      Swift_UVOT_int_V
%Aladin.Tree        Image/Optical/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-01TZ00:00:00Z

%ActionName         P-Swift-UVOT-int_WHITE.hpx
%Description        Combined Swift UVOT intensities: band WHITE
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/uvot/int/WHITE
%VerboseDescr       Intensity map for the Swift UVOT WHITE band for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/UVOT/int_WHITE
%Aladin.Profile     >6.1
%SkyFraction        0.002868
%Aladin.XLabel      Swift_UVOT_int_WHITE
%Aladin.Tree        Image/UV/Swift/UVOT
%Aladin.HpxParam    9 image equatorial fits png
%Aladin.Date        2017-09-01TZ00:00:00Z

%ActionName         P-Swift-XRT-exp.hpx
%Description        Combined Swift XRT exposure
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                https://skyview.gsfc.nasa.gov/surveys/xrt/int/all2
%VerboseDescr       Summed exposure for the Swift XRT for the period from 2005 through mid 2017
%Copyright          Generated from public data in HEASARC archive
%Origin             nasa.heasarc
%Id                 P/Swift/XRT/exp
%Aladin.Profile     >6.1
%SkyFraction        0.1907
%Aladin.XLabel      Swift_XRT_exp
%Aladin.Tree        Image/Xray/Swift/XRT
%Aladin.HpxParam    8 image equatorial fits png
%Aladin.Date        2017-09-01TZ00:00:00Z

%ActionName         P-TGSSADR.hpx
%Description        The TIFR GMRT Sky Survey, Alternative Data Release
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1465811895  2016/06/13 11:58:15
%Url                http://tgssadr.strw.leidenuniv.nl/hips/
%VerboseDescr       150 MHz radio intensity images of the sky above -53 degrees DEC. Note that this current release is an alpha version subject to change. Most likely anticipated changes are: (1) image rescaling, (2) addition of missing fields, (3) replacement of bad fields.
%Copyright          TGSS ADR webpage
%Origin             Leiden
%Id                 P/TGSSADR
%Aladin.Profile     >6.1 beta
%Copyright.Url      http://tgssadr.strw.leidenuniv.nl/
%SkyFraction        0.895
%Aladin.XLabel      TGSS ADR intensity maps (150 MHz)
%Aladin.Tree        Image/Radio
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2016-03-08T15:11Z

%ActionName         P-Tethys-Cassini-PIA18439.hpx
%Description        Tethys Cassini-PIA18439
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Tethys_Cassini-PIA18439
%VerboseDescr       This set of global, color mosaics of Saturn's moon Tethys was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system. These are the first global color maps of these moons produced from the Cassini data. he most obvious feature on the maps is the difference in color and brightness between the two hemispheres. The darker colors on the trailing hemispheres are thought to be due to alteration by magnetospheric particles and radiation striking those surfaces. The lighter-colored leading hemisphere is coated with icy dust from Saturn's E-ring, formed from tiny particles ejected from Enceladus' south pole. These satellites are all being painted by material erupted by neighboring Enceladus. The colors shown in these global mosaics are enhanced, or broader, relative to human vision, extending into the ultraviolet and infrared range. Resolution on Tethys in the maps is 250 meters per pixel. Image selection, radiometric calibration, geographic registration and photometric correction, as well as mosaic selection and assembly were performed by Paul Schenk at the Lunar and Planetary Institute. Original image planning and targeting for Saturn's icy moons were performed by Tilman Denk (Frei Universitat, Berlin) and Paul Helfenstein (Cornell University, Ithaca, New York). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.
%Copyright          JPL/PhotoJournal
%Origin             CDS
%Id                 P/Tethys/Cassini-PIA18439
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Tethys/Cassini-PIA18439
%Aladin.Tree        Solar system/Saturn/Tethys
%Aladin.HpxParam    3 image color tethys jpeg
%Aladin.Date        2018-01-24T13:30Z

%ActionName         P-Titan-ISS-P19658-4km.hpx
%Description        Titan ISS-P19658-4km
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Titan_ISS-P19658-4km
%VerboseDescr       This global digital map of Saturn's moon Titan was created using images taken by the Cassini spacecraft's imaging science subsystem (ISS). The map was produced in June 2015 using data collected through Cassini's flyby on April 7, 2014, known as "T100".
%Copyright          Planetary Data System, from USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Titan/ISS-P19658-4km
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Titan/ISS-P19658-4km
%Aladin.Tree        Solar system/Saturn/Titan
%Aladin.HpxParam    3 image color titan jpeg
%Aladin.Date        2018-01-21T11:06Z

%ActionName         P-Titan-SAR-HiSAR-128ppd.hpx
%Description        Titan SAR-HiSAR-128ppd
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Titan_SAR-HiSAR-128ppd
%VerboseDescr       Global map of Titan?s surface showing the coverage derived from Synthetic Aperture Radar (SAR) and High Altitude Synthetic Aperture Radar (HiSAR) images. This mosaic merges Cassini swaths through flyby T104 into a single mosaic. This is a preliminary product. The Cassini Titan Radio Detection and Ranging (RADAR) Mapper plays a significant role in investigating the surface of Titan. This multi-mode radar instrument operates in the 13.8 GHz Ku-band (or 2.2 cm wavelength) and is designed to probe the optically inaccessible surface of Titan. The four different modes of the instrument Synthetic Aperture Radar (SAR) imaging, Altimetry, Scatterometry and Radiometry allow surface imaging as well as topographic mapping at spacecraft altitudes between 100,000 km and about 1,000 km, with resolutions for the modes ranging from 100 s of km to a few hundred meters (Elachi et al. 2005) . The observations, particularly when performed in the active modes of SAR, altimetry and scatterometry, are largely unaffected by atmospheric contributions.
%Copyright          Planetary Data System, from USGS Astrogeology Science Center
%Origin             CDS
%Id                 P/Titan/SAR-HiSAR-128ppd
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Titan/SAR-HiSAR-128ppd
%Aladin.Tree        Solar system/Saturn/Titan
%Aladin.HpxParam    4 image color titan jpeg
%Aladin.Date        2018-01-21T11:02Z

%ActionName         P-Titania-Voyager.hpx
%Description        Titania Voyager
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Titania_Voyager
%VerboseDescr       Titania Uranus satellite map mosaicked with Voyager imagery by USGS
%Copyright          Caltech/JPL/NASA
%Origin             CDS
%Id                 P/Titania/Voyager
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Titania/Voyager
%Aladin.Tree        Solar system/Uranus/Titania
%Aladin.HpxParam    3 image color titania jpeg
%Aladin.Date        2018-01-31T06:36Z

%ActionName         P-Triton-Voyager2-600m.hpx
%Description        Triton Voyager2-600m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Triton_Voyager2-600m
%VerboseDescr       The Voyager 2 spacecraft flew by Triton, a moon of Neptune, in the summer of 1989. Dr. Paul Schenk, a scientist at the Lunar and Planetary Institute in Houston, used Voyager data to construct the best-ever global color map of Triton. This map has a resolution of 1,970 feet (600 meters) per pixel. The colors have been enhanced to bring out contrast but are a close approximation to Triton's natural colors. Voyager's "eyes" saw in colors slightly different from human eyes, and this map was produced using orange, green and blue filter images. The Voyager mission is managed by NASA's Jet Propulsion Laboratory, in Pasadena, California, for NASA's Science Mission Directorate (SMD) at NASA Headquarters in Washington. Caltech manages JPL for NASA.
%Copyright          Was originally released in the PDS Photojpurnal as file PIA18668.tif
%Origin             CDS
%Id                 P/Triton/Voyager2-600m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Triton/Voyager2-600m
%Aladin.Tree        Solar system/Neptune/Triton
%Aladin.HpxParam    3 image color triton jpeg
%Aladin.Date        2018-01-23T13:52Z

%ActionName         P-UHSDR1-J.hpx
%Description        UHS DR1 J
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://surveys.roe.ac.uk/hips71/UHS/UHSDR1_PIX
%VerboseDescr       UKIRT Hemisphere Survey, UHS DR1 J-band WFCAM
%Origin             wfau.roe.ac.uk
%Id                 P/UHSDR1/J
%Aladin.Profile     >6.1
%SkyFraction        0.3083
%Aladin.XLabel      UKIRT Hemisphere Survey DR1 J
%Aladin.Tree        Image/Infrared/UKIRT-WFCAM
%Aladin.HpxParam    10 image equatorial png fits
%Aladin.Date        2018-10-16T12:41Z

%ActionName         P-ULTRAVISTA-H.hpx
%Description        ULTRAVISTA H
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/H
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/H
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        6.103E-5
%Aladin.XLabel      ULTRAVISTA H
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-03
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2013-06-21T11:25Z

%ActionName         P-ULTRAVISTA-J.hpx
%Description        ULTRAVISTA J
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/J
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/J
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        6.103E-5
%Aladin.XLabel      ULTRAVISTA J
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-02
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2013-06-21T14:40Z

%ActionName         P-ULTRAVISTA-Ks.hpx
%Description        ULTRAVISTA Ks
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/Ks
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/Ks
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        6.103E-5
%Aladin.XLabel      ULTRAVISTA Ks
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-04
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2013-06-21T16:14Z

%ActionName         P-ULTRAVISTA-NB118.hpx
%Description        ULTRAVISTA NB118
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/NB118
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/NB118
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        5.213E-5
%Aladin.XLabel      ULTRAVISTA NB118
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-05
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2013-06-21T17:43Z

%ActionName         P-ULTRAVISTA-Y.hpx
%Description        ULTRAVISTA Y
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/Y
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/Y
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        6.103E-5
%Aladin.XLabel      ULTRAVISTA Y
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-01
%Aladin.HpxParam    12 image equatorial jpeg fits
%Aladin.Date        2013-06-21T13:09Z

%ActionName         P-ULTRAVISTA-color-YJKs.hpx
%Description        ULTRAVISTA color YJKs
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/UltraVista/ColorYJKs
%VerboseDescr       UltraVISTA is an Ultra Deep, near-infrared survey with the new VISTA surveys telescope of the European Southern Observatory (ESO). Over the course of 5 years, UltraVISTA will repeatedly image the COSMOS field in 5 bands covering a 1.5deg^2 field.
%Copyright          ULTRAVISTA consortium
%Origin             CDS
%Id                 P/ULTRAVISTA/color/YJKs
%Aladin.Profile     >6.1
%Copyright.Url      http://home.strw.leidenuniv.nl/~ultravista/
%SkyFraction        4.519E-5
%Aladin.XLabel      ULTRAVISTA color YJKs
%Aladin.Tree        Image/Infrared/UltraVista
%Aladin.MenuNumber  04-002-00
%Aladin.HpxParam    12 image color equatorial jpeg
%Aladin.Date        2013-06-25T10:36Z

%ActionName         P-URUMQI-POLQ.hpx
%Description        URUMQI POLQ
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/URUMQI_POLQ
%VerboseDescr       6cm polarization survey (Stokes Q) of the Galactic Plane (10°<l<230° and |b|<5°) using the Urumqi 25-m telescope, at an angular resolution of 9.5?.Units:microKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/URUMQI/POLQ
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05604
%Aladin.XLabel      Urumqi 6cm POLQ
%Aladin.Tree        Image/Radio/Urumqi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-05T12:14Z

%ActionName         P-URUMQI-POLU.hpx
%Description        URUMQI POLU
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/URUMQI_POLU
%VerboseDescr       6cm polarization survey (Stokes U) of the Galactic Plane (10°<l<230° and |b|<5°) using the Urumqi 25-m telescope, at an angular resolution of 9.5?.Units:microKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/URUMQI/POLU
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05604
%Aladin.XLabel      Urumqi 6cm POLU
%Aladin.Tree        Image/Radio/Urumqi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-05T12:16Z

%ActionName         P-URUMQI.hpx
%Description        URUMQI
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/URUMQI_I
%VerboseDescr       6cm survey of the Galactic Plane (10°<l<230° and |b|<5°) using the Urumqi 25-m telescope, at an angular resolution of 9.5?.Units:microKTB.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/URUMQI
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.05605
%Aladin.XLabel      Urumqi 6cm intensity
%Aladin.Tree        Image/Radio/Urumqi
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-12-05T12:17Z

%ActionName         P-Umbriel-Voyager.hpx
%Description        Umbriel Voyager
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Umbriel_Voyager
%VerboseDescr       Umbriel Uranus satellite map mosaicked with Voyager imagery by USGS
%Copyright          Caltech/JPL/NASA
%Origin             CDS
%Id                 P/Umbriel/Voyager
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Umbriel/Voyager
%Aladin.Tree        Solar system/Uranus/Umbriel
%Aladin.HpxParam    3 image color umbriel jpeg
%Aladin.Date        2018-01-31T06:36Z

%ActionName         P-VISTA-VIKING-H.hpx
%Description        VISTA VIKING H
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VIKING/VISTA-VIKING-H
%VerboseDescr       The VIKING (VISTA Kilo-degree Infrared Galaxy) survey is a medium-deep survey of 1500 square degrees over two areas of the extra-galactic sky with VISTA in zYJHKs bands to sample the restframe optical for galaxies at z>1. The VIKING survey area is split into two areas: an equatorial strip between right ascension 9 and 15.8 hours and 8 degrees wide; and a strip over the South Galactic Pole between right ascension 22 and 3.5 hours and 10 degrees wide.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VIKING/H
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.02492
%Aladin.XLabel      VISTA VIKING H
%Aladin.Tree        Image/Infrared/VISTA/VIKING
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-04-23T01:45Z

%ActionName         P-VISTA-VIKING-J.hpx
%Description        VISTA VIKING J
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VIKING/VISTA-VIKING-J
%VerboseDescr       The VIKING (VISTA Kilo-degree Infrared Galaxy) survey is a medium-deep survey of 1500 square degrees over two areas of the extra-galactic sky with VISTA in zYJHKs bands to sample the restframe optical for galaxies at z>1. The VIKING survey area is split into two areas: an equatorial strip between right ascension 9 and 15.8 hours and 8 degrees wide; and a strip over the South Galactic Pole between right ascension 22 and 3.5 hours and 10 degrees wide.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VIKING/J
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.02438
%Aladin.XLabel      VISTA VIKING J
%Aladin.Tree        Image/Infrared/VISTA/VIKING
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-07-11T17:04Z

%ActionName         P-VISTA-VIKING-K.hpx
%Description        VISTA VIKING K
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VIKING/VISTA-VIKING-K
%VerboseDescr       The VIKING (VISTA Kilo-degree Infrared Galaxy) survey is a medium-deep survey of 1500 square degrees over two areas of the extra-galactic sky with VISTA in zYJHKs bands to sample the restframe optical for galaxies at z>1. The VIKING survey area is split into two areas: an equatorial strip between right ascension 9 and 15.8 hours and 8 degrees wide; and a strip over the South Galactic Pole between right ascension 22 and 3.5 hours and 10 degrees wide.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VIKING/K
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.0249
%Aladin.XLabel      VISTA VIKING K
%Aladin.Tree        Image/Infrared/VISTA/VIKING
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-07-07T01:49Z

%ActionName         P-VISTA-VIKING-Y.hpx
%Description        VISTA VIKING Y
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VIKING/VISTA-VIKING-Y
%VerboseDescr       The VIKING (VISTA Kilo-degree Infrared Galaxy) survey is a medium-deep survey of 1500 square degrees over two areas of the extra-galactic sky with VISTA in zYJHKs bands to sample the restframe optical for galaxies at z>1. The VIKING survey area is split into two areas: an equatorial strip between right ascension 9 and 15.8 hours and 8 degrees wide; and a strip over the South Galactic Pole between right ascension 22 and 3.5 hours and 10 degrees wide.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VIKING/Y
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.02457
%Aladin.XLabel      VISTA VIKING Y
%Aladin.Tree        Image/Infrared/VISTA/VIKING
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-09-05T16:47Z

%ActionName         P-VISTA-VIKING-Z.hpx
%Description        VISTA VIKING Z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VIKING/VISTA-VIKING-Z
%VerboseDescr       The VIKING (VISTA Kilo-degree Infrared Galaxy) survey is a medium-deep survey of 1500 square degrees over two areas of the extra-galactic sky with VISTA in zYJHKs bands to sample the restframe optical for galaxies at z>1. The VIKING survey area is split into two areas: an equatorial strip between right ascension 9 and 15.8 hours and 8 degrees wide; and a strip over the South Galactic Pole between right ascension 22 and 3.5 hours and 10 degrees wide.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VIKING/Z
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.02466
%Aladin.XLabel      VISTA VIKING Z
%Aladin.Tree        Image/Infrared/VISTA/VIKING
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2018-09-14T19:02Z

%ActionName         P-VISTA-VVV-DR4-ColorJYZ.hpx
%Description        VISTA DR4 ColorJYZ
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-ColorJYZ
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/ColorJYZ
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.01373
%Aladin.XLabel      VISTA DR4 ColorJYZ
%Aladin.Tree        Image/Infrared/VISTA/VVV
%Aladin.HpxParam    11 image color equatorial png
%Aladin.Date        2017-12-18T11:42Z

%ActionName         P-VISTA-VVV-DR4-H-Bulge.hpx
%Description        VISTA VVV DR4 H Bulge
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-H-Bulge
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/H/Bulge
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.007661
%Aladin.XLabel      VISTA VVV DR4 H Bulge
%Aladin.Tree        Image/Infrared/VISTA
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2017-09-29T19:20Z

%ActionName         P-VISTA-VVV-DR4-H-Disk.hpx
%Description        VISTA VVV DR4 H Disk
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-H-Disk
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/H/Disk
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.006092
%Aladin.XLabel      VISTA VVV DR4 H Disk
%Aladin.Tree        Image/Infrared/VISTA
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2017-09-30T01:49Z

%ActionName         P-VISTA-VVV-DR4-J.hpx
%Description        VISTA VVV DR4 J
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-J
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/J
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.01373
%Aladin.XLabel      VISTA VVV DR4 J
%Aladin.Tree        Image/Infrared/VISTA/VVV
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2017-09-30T11:22Z

%ActionName         P-VISTA-VVV-DR4-Y.hpx
%Description        VISTA VVV DR4 Y
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-Y
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/Y
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.01373
%Aladin.XLabel      VISTA VVV DR4 Y
%Aladin.Tree        Image/Infrared/VISTA/VVV
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2017-10-01T21:42Z

%ActionName         P-VISTA-VVV-DR4-Z.hpx
%Description        VISTA VVV DR4 Z
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VVV_DR4/VISTA-VVV-DR4-Z
%VerboseDescr       The public ESO near-IR variability survey (VVV) scanned the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey took 1929 hours of observations with the 4-metre VISTA telescope during five years (2010-2014), covering ~10^9 point sources across an area of 520 deg^2, including 33 known globular clusters and ~350 open clusters. The final product is a deep near-IR atlas in five passbands (0.9-2.5 microns) and a catalogue of more than 10^6 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. The VISTA Variables in the Via Lactea (VVV) survey fourth data release (DR4) provides VISTA tile images and source lists in ZYJHKs filters, processed by the Cambridge Astronomical Survey Unit (CASU), for a total sky coverage of 560 square degrees. DR4 contains science data products from observations in the period 1 October 2013 ? 15 October 2015, and also science data products from observations in September 2010 to September 2013 not included in the previous release.
%Copyright          ESO
%Origin             CDS
%Id                 P/VISTA/VVV/DR4/Z
%Aladin.Profile     >6.1
%Copyright.Url      https://www.eso.org/sci/observing/policies/publications.html
%SkyFraction        0.01373
%Aladin.XLabel      VISTA VVV DR4 Z
%Aladin.Tree        Image/Infrared/VISTA/VVV
%Aladin.HpxParam    11 image equatorial png fits
%Aladin.Date        2017-09-30T22:16Z

%ActionName         P-VLSSr.hpx
%Description        VLSSr - 74 MHz continuum
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VLSSr
%VerboseDescr       The VLA Low-Frequency Sky Survey Redux (VLSS) is a 74 MHz continuum survey covering the entire sky north of -30 degrees declination. Using the VLA in BnA and B-configurations, it will map the entire survey region at a resolution of 80" and with an average rms noise of 0.1 Jy/beam. This version include the data from the VLSS redux which increased the coverage region slightly and substantially improved the data reduction. Details are in the Lane et al. (2012) reference. Frequency: 74 MHz, PixelUnits: Janskies/Beam. The VLSSr represents a major improvement to the original VLSS over most of the sky. It includes six previously unpublished fields, and improved dynamic range in 95% of all fields. The clean bias has been halved and is now 0.66 times the local RMS. The largest angular size imaged has been roughly doubled to 36', and the number of cataloged sources is increased by 35% to %93,000.
%Copyright          NRAO & The NRL
%Origin             CDS
%Id                 P/VLSSr
%Aladin.Profile     >6.1
%Copyright.Url      http://www.cv.nrao.edu/vlss/findFITS.shtml
%SkyFraction        0.7463
%Aladin.XLabel      VLSSr
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-10
%Aladin.HpxParam    5 image equatorial png fits
%Aladin.Date        2014-12-16T10:19Z

%ActionName         P-VTSS-CONT.hpx
%Description        Virginia Tech Spectral-Line Survey (VTSS) - Continuum corrected Halpha image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/VTSS_CONT
%VerboseDescr       Continuum corrected Halpha, using the Virginia Tech Spectral-Line Imaging Camera (SLIC). The resolution of the map is 1.6? and units are Rayleighs.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/VTSS/CONT
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.181
%Aladin.XLabel      VTSS CONT
%Aladin.Tree        Image/Gas-lines/Halpha/VTSS
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2018-03-12T15:46Z

%ActionName         P-VTSS-Ha.hpx
%Description        Virginia Tech Spectral-Line Survey (VTSS) - Halpha image
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/VTSS
%VerboseDescr       6563 A H-alpha recombination line of Hydrogen, using the Virginia Tech Spectral-Line Imaging Camera (SLIC). The resolution of the map is 1.6? and units are Rayleighs.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/VTSS/Ha
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        0.1918
%Aladin.XLabel      VTSS Halpha
%Aladin.Tree        Image/Gas-lines/Halpha/VTSS
%Aladin.MenuNumber  lite
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2018-03-12T14:53Z

%ActionName         P-VTSS-HaCC.hpx
%Description        VTSS HaCC - Continuum corrected Halpha
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VTSS/HaCC
%VerboseDescr       The VTSS is a wide-field image survey of the Galaxy's warm ionized interstellar medium (WIM, a 10,000 K plasma). The instrumentation used is the Virginia Tech Spectral Line Imaging Camera (SLIC), specially designed for obtaining sensitive, arcminute-resolution, 10-degree wide images of the 6563Å H-alpha recombination line of hydrogen, and the [SII]6717,6731Å doublet emission of singly ionized sulfur. This survey cover the northern hemisphere (declinations greater than -15 degrees).
%Copyright          (c) Virginia Tech Physics - HEALPixed by CDS
%Origin             CDS
%Id                 P/VTSS/HaCC
%Aladin.Profile     >6.1
%Copyright.Url      http://www.phys.vt.edu/~halpha/
%SkyFraction        0.3164
%Aladin.XLabel      VTSS HaCC
%Aladin.Tree        Image/Gas-lines/Halpha/VTSS
%Aladin.MenuNumber  06-03-02
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-04-19T18:08Z

%ActionName         P-Venus-Magellan-C3-MDIR-2025m.hpx
%Description        Magellan Global C3-MDIR Mosaic 2025m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Venus_Magellan_C3-MDIR-2025m
%VerboseDescr       The original Magellan Compressed Mosaicked Image Data Record (C3-MIDR) archive contains three times compressed mosaics of image swaths (C-BIDRs) at a resolution of 2025 m/pixel. C3-MIDRs consist of mosaics generated by computing 3x3 pixel arithmetic moving averages from the C2-MIDRs. C3-MIDRs, with their 2.025 km pixel widths, are designed to cover the planet at reasonably high resolution and high signal to noise ratio.
%Copyright          Public domain
%Origin             CDS
%Id                 P/Venus/Magellan/C3-MDIR-2025m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Venus Magellan Global Mosaic
%Aladin.Tree        Solar system/Venus
%Aladin.HpxParam    3 image venus png fits
%Aladin.Date        2017-11-14T16:48Z

%ActionName         P-Venus-Magellan-C3-MDIR-ClrTopo-6600m-color.hpx
%Description        Venus Magellan C3-MDIR-ClrTopo-6600m-color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Venus_Magellan_C3-MDIR-ClrTopo-6600m-color
%Copyright          USGS (https://astrogeology.usgs.gov/), intermediate FITS by Chiara Marmo
%Origin             CDS
%Id                 P/Venus/Magellan/C3-MDIR-ClrTopo-6600m-color
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      P/Venus/Magellan/C3-MDIR-ClrTopo-6600m-color
%Aladin.Tree        Solar system/Venus
%Aladin.HpxParam    3 image color venus jpeg
%Aladin.Date        2017-11-14T14:40Z

%ActionName         P-Venus-Magellan-MeterScaleSlope-4641m.hpx
%Description        Venus Magellan MeterScaleSlope-4641m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Venus_Magellan_MeterScaleSlope-4641m
%VerboseDescr       Global Slope Data Record (GSDR). The surface meter-scale slopes are derived by fitting altimeter echoes from the fan-beam altimetry antenna as a function of time to Hagfors' radar backscatter model templates. The data are then re-sampled at a resolution of about 5x5 kilometers per pixel. Each GSDR image pixel is represented by a 8-bit unsigned integer. Pixels lying outside the domain of the projection are set to NoData (0). In all images, pixels with unknown or unmeasured values are also set to NoData. The remaining values are related to the slope by the following equation: DN = ((SLOPE ) * 10) + 1 .
%Copyright          public domain, please cite authors
%Origin             CDS
%Id                 P/Venus/Magellan/MeterScaleSlope-4641m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Venus Magellan Global Mosaic
%Aladin.Tree        Solar system/Venus
%Aladin.HpxParam    3 image venus png fits
%Aladin.Date        2017-11-14T17:01Z

%ActionName         P-Venus-Magellan-Microwave-Emissivity-4641m.hpx
%Description        Venus Magellan Microwave-Emissivity-4641m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Venus_Magellan_Microwave-Emissivity-4641m
%VerboseDescr       Global Emissivity Data Record (GEDR). The emissivity of a surface is defined as the thermal power emitted by that surface divided by the power emitted by a black body of the same size and at the same physical temperature. The polarization direction is horizontal (E-field tangential to surface), and the emissivity is not corrected for emission angle or surface roughness or tilt. This data set includes all Magellan measurements in which the high-gain antenna followed the nominal look-angle profile, in which the observed emission angle varied from 48 degrees off the local vertical at periapsis (ca. 10N latitude) to 15 degrees off vertical at the 90N and 70S. To make the GEDR images, Magellan radiometer data, in the form of readings of antenna noise temperature, are corrected for antenna sidelobe effects and for emission and absorption by the Venus atmosphere. The component reflected from the surface is modeled as a specular reflection with power reflection coefficient equal to (1 - emissivity). The location and planetary radius at the antenna boresight intercept point are derived from GTDR images and the physical surface temperature is calculated using the adiabatic model of Kliore et al., 1985. The data are then filtered to remove low-frequency instrument calibration errors, and re-sampled at a resolution of about 5x5 kilometers per pixel.
%Copyright          public domain, please cite authors
%Origin             CDS
%Id                 P/Venus/Magellan/Microwave-Emissivity-4641m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Venus Magellan Global Mosaic
%Aladin.Tree        Solar system/Venus
%Aladin.HpxParam    3 image venus png fits
%Aladin.Date        2017-11-14T17:18Z

%ActionName         P-Venus-Magellan-Topography-4641m.hpx
%Description        Venus Magellan Topography-4641m
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Planets/CDS_P_Venus_Magellan_Topography-4641m
%VerboseDescr       This product has been superseeded by version2:https://astrogeology.usgs.gov/search/map/Venus/Magellan/RadarProperties/Venus_Magellan_Topography_Global_4641m_v02
%Copyright          USGS (https://astrogeology.usgs.gov/), intermediate FITS by Chiara Marmo
%Origin             CDS
%Id                 P/Venus/Magellan/Topography-4641m
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Venus Magellan Global Mosaic
%Aladin.Tree        Solar system/Venus
%Aladin.HpxParam    3 image venus png fits
%Aladin.Date        2017-11-14T16:43Z

%ActionName         P-VistaOrion-color.hpx
%Description        VISTA Orion A color
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/VISTA/VISTA-Orion-A-Colored
%VerboseDescr       The  observations of the Orion A molecular cloud have been carried out with the Visible and Infrared Survey Telescope for Astronomy, a 4m class telescope that is operated by the European Southern Observatory (ESO) as part of its Cerro Paranal facilities. The HEALPix survey, color (R=red[1.25um]/G=green[1.65um]/B=blue[2.15um]) is based on near-infrared data obtained with the ESO VISTA telescope. Program ID: 090.C-0797(A)
%Copyright          ESO
%Origin             CDS
%Id                 P/VistaOrion/color
%Aladin.Profile     >6.1
%Copyright.Url      http://www.eso.org/public/
%SkyFraction        5.337E-4
%Aladin.XLabel      Vista Orion A color
%Aladin.Tree        Image/Infrared/VISTA
%Aladin.HpxParam    9 image color equatorial png
%Aladin.Date        2015-12-16T12:56Z

%ActionName         P-WENSS.hpx
%Description        The Westerbork Northern Sky Survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WENSS
%VerboseDescr       WENSS radio survey (325MHz). Resampled in Healpix by CDS. The Westerbork Northern Sky Survey (WENSS) is a low-frequency radio survey, designed to cover the whole sky north of declination 30deg at a wavelength of 92 cm (325  MHz), and about a quarter of this region, concentrated at high galactic latitudes, at a wavelength of 49 cm (609  MHz), to a limiting flux density of approximately 18 mJy and 15 mJy respectively. Observations for WENSS were carried out with the WSRT (The Westerbork Synthesis Radio Telescope) in a standard  set-up.
%Copyright          https://heasarc.gsfc.nasa.gov/w3browse/all/wenss.html
%Origin             CDS
%Id                 P/WENSS
%Aladin.Profile     >6.1
%Copyright.Url      http://www.astron.nl/wow/testcode.php?survey=1
%SkyFraction        0.2684
%Aladin.XLabel      WENSS
%Aladin.Tree        Image/Radio
%Aladin.MenuNumber  05-09
%Aladin.HpxParam    5 image equatorial png jpeg fits
%Aladin.Date        2014-04-17T21:27Z

%ActionName         P-WHAM.hpx
%Description        WHAM Halpha
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://cade.irap.omp.eu/documents/Ancillary/4Aladin/WHAM
%VerboseDescr       6563 A H-alpha recombination line of Hydrogen, from the Wisconsin Halpha Mapper (WHAM) all-sky survey. The resolution of the map is 1 degree and units are Rayleighs.\nHealpix map built by D. Paradis (IRAP/CADE)
%Copyright          IRAP/CADE
%Origin             ov-gso
%Id                 P/WHAM
%Aladin.Profile     >6.1
%Copyright.Url      http://cade.irap.omp.eu
%SkyFraction        1
%Aladin.XLabel      WHAM Halpha
%Aladin.Tree        Image/Gas-lines/Halpha
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2017-05-15T12:44Z

%ActionName         P-WISE-W1.hpx
%Description        WISE W1 (3.4um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WISE/W1
%VerboseDescr       Wide-field Infrared Survey Explore (WISE) is a MIDEX (medium class Explorer) mission funded by NASA. The WISE short-wavelength channels employ 4.2 and 5.4um cutoff HgCdTe arrays fabricated by Teledyne Imaging Sensors with 1024x1024 pixels each 18 um square. WISE W1 (3.4um) from raw Atlas Images (not background matched nor zodi-corrected). Resampled in Healpix by Frank Masci (IPAC). The spatial resolution is limited to 12 arcsec.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/WISE/W1
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      WISE W1
%Aladin.Tree        Image/Infrared/WISE/Low
%Aladin.MenuNumber  04-003-XX-01
%Aladin.HpxParam    5 image galactic jpeg fits
%Aladin.Date        2012-04-05T13:30Z

%ActionName         P-WISE-W2.hpx
%Description        WISE W2 (4.6um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WISE/W2
%VerboseDescr       Wide-field Infrared Survey Explore (WISE) is a MIDEX (medium class Explorer) mission funded by NASA. The WISE short-wavelength channels employ 4.2 and 5.4um cutoff HgCdTe arrays fabricated by Teledyne Imaging Sensors with 1024x1024 pixels each 18 um square. WISE W2 (4.6um) from raw Atlas Images (not background matched nor zodi-corrected).Resampled in Healpix by Frank Masci (IPAC). The spatial resolution is limited to 12 arcsec.
%Copyright          University of Massachusetts & IPAC/Caltech
%Origin             CDS
%Id                 P/WISE/W2
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      WISE W2
%Aladin.Tree        Image/Infrared/WISE/Low
%Aladin.MenuNumber  04-003-XX-02
%Aladin.HpxParam    5 image galactic jpeg fits
%Aladin.Date        2015-04-13T15:21Z

%ActionName         P-WISE-W3.hpx
%Description        WISE W3 (12um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WISE/W3
%VerboseDescr       Wide-field Infrared Survey Explore (WISE) is a MIDEX (medium class Explorer) mission funded by NASA. The WISE short-wavelength channels employ 4.2 and 5.4um cutoff HgCdTe arrays fabricated by Teledyne Imaging Sensors with 1024x1024 pixels each 18 um square. WISE W3 (12um) from raw Atlas Images (not background matched nor zodi-corrected). Resampled in Healpix by Frank Masci (IPAC). The spatial resolution is limited to 12 arcsec.
%Copyright          WISE acknowledgment
%Origin             CDS
%Id                 P/WISE/W3
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      WISE W3
%Aladin.Tree        Image/Infrared/WISE/Low
%Aladin.MenuNumber  04-003-XX-03
%Aladin.HpxParam    5 image galactic jpeg fits
%Aladin.Date        2015-04-13T15:42Z

%ActionName         P-WISE-W4.hpx
%Description        WISE W4 (22um)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WISE/W4
%VerboseDescr       Wide-field Infrared Survey Explore (WISE) is a MIDEX (medium class Explorer) mission funded by NASA. The WISE short-wavelength channels employ 4.2 and 5.4um cutoff HgCdTe arrays fabricated by Teledyne Imaging Sensors with 1024x1024 pixels each 18 um square. WISE W1 (3.4um) from raw Atlas Images (not background matched nor zodi-corrected). Resampled in Healpix by Frank Masci (IPAC). The spatial resolution is limited to 12 arcsec.
%Copyright          WISE acknowledgment
%Origin             CDS
%Id                 P/WISE/W4
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      WISE W4
%Aladin.Tree        Image/Infrared/WISE/Low
%Aladin.MenuNumber  04-003-XX-04
%Aladin.HpxParam    5 image galactic jpeg fits
%Aladin.Date        2015-04-13T16:04Z

%ActionName         P-WISE-WSSA-12um.hpx
%Description        Diffuse dust 12um WSSA (Meisner & Finkbeiner 2013)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WSSA
%VerboseDescr       Diffuse Galactic dust emission at 12um from the processing of the Wide-field Infrared Survey Explorer (WISE) data set by Meisner & Finkbeiner (2013). The 430 WISE Sky Survey Atlas (WSSA) tiles were resampled in Healpix by Thomas Boch (CDS). The spatial resolution is limited to 15 arcsec.
%Copyright          Meisner & Finkbeiner (2013)
%Origin             CDS
%Id                 P/WISE/WSSA/12um
%Aladin.Profile     >6.1
%Copyright.Url      http://faun.rc.fas.harvard.edu/ameisner/wssa/
%SkyFraction        1
%Aladin.XLabel      WISE WSSA 12um
%Aladin.Tree        Image/Infrared/WISE/WSSA
%Aladin.MenuNumber  04-003-01-01
%Aladin.HpxParam    7 image equatorial jpeg fits
%Aladin.Date        2014-04-17T22:08Z

%ActionName         P-WMAP-K-9yr.hpx
%Description        WMAP K - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WMAP9yr/WMAPK9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The K-band is centered at 13 mm (23 GHz), its beam size is 0.88 deg (square-root of the beam solid angle).
%Copyright          HEASARC/LAMBDA
%Origin             CDS
%Id                 P/WMAP/K/9yr
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%SkyFraction        1
%Aladin.XLabel      WMAP K 9yr
%Aladin.Tree        Image/Radio/WMAP
%Aladin.MenuNumber  05-03-05
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-11-25T18:10Z

%ActionName         P-WMAP-Ka-9yr.hpx
%Description        WMAP Ka - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WMAP9yr/WMAPKa9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The Ka-band is centered at 9.1 mm (33 GHz), its beam size is 0.66 deg (square-root of the beam solid angle).
%Copyright          HEASARC/LAMBDA
%Origin             CDS
%Id                 P/WMAP/Ka/9yr
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%SkyFraction        1
%Aladin.XLabel      WMAP Ka 9yr
%Aladin.Tree        Image/Radio/WMAP
%Aladin.MenuNumber  05-03-04
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-11-25T18:12Z

%ActionName         P-WMAP-Q-9yr.hpx
%Description        WMAP Q - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WMAP9yr/WMAPQ9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The Q-band is centered at 7.3 mm (41 GHz), its beam size is 0.51 deg (square-root of the beam solid angle).
%Copyright          HEASARC/LAMBDA
%Origin             CDS
%Id                 P/WMAP/Q/9yr
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%SkyFraction        1
%Aladin.XLabel      WMAP Q 9yr
%Aladin.Tree        Image/Radio/WMAP
%Aladin.MenuNumber  05-03-03
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-11-25T18:14Z

%ActionName         P-WMAP-V-9yr.hpx
%Description        WMAP V - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WMAP9yr/WMAPV9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The V-band is centered at 4.9 mm (61 GHz), its beam size is 0.35 deg (square-root of the beam solid angle).
%Copyright          HEASARC/LAMBDA
%Origin             CDS
%Id                 P/WMAP/V/9yr
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%SkyFraction        1
%Aladin.XLabel      WMAP V 9yr
%Aladin.Tree        Image/Radio/WMAP
%Aladin.MenuNumber  05-03-02
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-11-25T18:15Z

%ActionName         P-WMAP-W-9yr.hpx
%Description        WMAP W - 9yr
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/WMAP9yr/WMAPW9yr
%VerboseDescr       The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The W-band is centered at 3.2 mm (94 GHz), its beam size is 0.22 deg (square-root of the beam solid angle).
%Copyright          HEASARC/LAMBDA
%Origin             CDS
%Id                 P/WMAP/W/9yr
%Aladin.Profile     >6.1
%Copyright.Url      http://lambda.gsfc.nasa.gov/product/map/dr5/maps_band_r9_i_9yr_get.cfm
%SkyFraction        1
%Aladin.XLabel      WMAP W 9yr
%Aladin.Tree        Image/Radio/WMAP
%Aladin.MenuNumber  05-03-01
%Aladin.HpxParam    3 image galactic png jpeg fits
%Aladin.Date        2014-11-25T18:16Z

%ActionName         P-XMM-PN-color.hpx
%Description        False color X-ray images (Red=0.5-1 Green=1-2 Blue=2-4.5 Kev )
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-XMM-PN-color_0.hpx availability=9999
%SeeAction          P-XMM-PN-color_1.hpx availability=0
%SeeAction          P-XMM-PN-color_2.hpx availability=9999
%SeeAction          P-XMM-PN-color_3.hpx availability=9999
%VerboseDescr       Colored image made with all PN images of the 3xmmdr8: Red=0.5-1Kev Green=1-2Kev  Blue=2-4.5Kev - Healpixilized by Michel L. [Observatoire de Strasbourg]
%Copyright          (c) ESA / SSC XMM-Newton
%Origin             xcatdb
%Id                 P/XMM/PN/color
%Aladin.Profile     >6.1
%Copyright.Url      http://xmmssc.irap.omp.eu/
%SkyFraction        0.08287
%Aladin.XLabel      XMM PN colored
%Aladin.Tree        Image/X-ray/XMM
%Aladin.MenuNumber  lite
%Aladin.HpxParam    7 image color equatorial png
%Aladin.Date        2018-07-10T06:48Z

%ActionName         P-XMM-PN-eb2.hpx
%Description        X-ray images on band 0.5-1Kev
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://saada.unistra.fr/PNRed
%VerboseDescr       Image made with all PN images of the 3xmmdr8 in band 0.5-1Kev - Healpixilized by L. Michel [Observatoire de Strasbourg]
%Copyright          (c) ESA / SSC XMM-Newton
%Origin             xcatdb
%Id                 P/XMM/PN/eb2
%Aladin.Profile     >6.1
%Copyright.Url      http://xmmssc.irap.omp.eu/
%SkyFraction        0.02227
%Aladin.XLabel      XMM PN eb2
%Aladin.Tree        Image/X-ray/XMM
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2018-07-09T16:14Z

%ActionName         P-XMM-PN-eb3.hpx
%Description        X-ray images on band 1-2Kev
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://saada.unistra.fr/PNGreen
%VerboseDescr       Image made with all PN images of the 3xmmdr8 in band 1-2Kev - Healpixilized by L. Michel [Observatoire de Strasbourg]
%Copyright          (c) ESA / SSC XMM-Newton
%Origin             xcatdb
%Id                 P/XMM/PN/eb3
%Aladin.Profile     >6.1
%Copyright.Url      http://xmmssc.irap.omp.eu/
%SkyFraction        0.02227
%Aladin.XLabel      P/XMM/PN/eb3
%Aladin.Tree        Image/X-ray/XMM
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2018-07-09T17:43Z

%ActionName         P-XMM-PN-eb4.hpx
%Description        X-ray images on band 2-4.5Kev
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://saada.unistra.fr/PNBlue
%VerboseDescr       Image made with all PN images of the 3xmmdr8 in band 2-4.5Kev - Healpixilized by L. Michel [Observatoire de Strasbourg]
%Copyright          (c) ESA / SSC XMM-Newton
%Origin             xcatdb
%Id                 P/XMM/PN/eb4
%Aladin.Profile     >6.1
%Copyright.Url      http://xmmssc.irap.omp.eu/
%SkyFraction        0.02227
%Aladin.XLabel      XMM PN eb4
%Aladin.Tree        Image/X-ray/XMM
%Aladin.HpxParam    7 image equatorial png fits
%Aladin.Date        2018-07-09T19:15Z

%ActionName         P-allWISE-W1.hpx
%Description        AllWISE W1 (3.4um) from raw Atlas Images
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/AllWISE/W1
%VerboseDescr       NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al.2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5 sigma point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.
%Copyright          IPAC/NASA
%Origin             CDS
%Id                 P/allWISE/W1
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/
%SkyFraction        1
%Aladin.XLabel      The Wide-field Infrared Survey Explorer - W1 band (allWISE W1)
%Aladin.Tree        Image/Infrared/WISE
%Aladin.MenuNumber  04-003-01
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2016-06-03T14:49Z

%ActionName         P-allWISE-W2.hpx
%Description        AllWISE W2 (4.6um) from raw Atlas Images
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/AllWISE/W2
%VerboseDescr       NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al.2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5 sigma point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.
%Copyright          IPAC/NASA
%Origin             CDS
%Id                 P/allWISE/W2
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allwise/expsup/sec1_6b.html
%SkyFraction        1
%Aladin.XLabel      The Wide-field Infrared Survey Explorer - W2 band (allWISE W2)
%Aladin.Tree        Image/Infrared/WISE
%Aladin.MenuNumber  04-003-02
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2016-06-03T14:58Z

%ActionName         P-allWISE-W3.hpx
%Description        AllWISE W3 (12um) from raw Atlas Images
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/AllWISE/W3
%VerboseDescr       NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al.2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5 sigma point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.
%Copyright          IPAC/NASA
%Origin             CDS
%Id                 P/allWISE/W3
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allwise/expsup/sec1_6b.html
%SkyFraction        0.9999
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%Aladin.MenuNumber  04-003-03
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2016-06-03T14:58Z

%ActionName         P-allWISE-W4.hpx
%Description        AllWISE W4 (22um) from raw Atlas Images
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1530785658  2018/07/05 12:14:18
%Url                http://alasky.u-strasbg.fr/AllWISE/W4
%VerboseDescr       NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al.2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5 sigma point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.
%Copyright          IPAC/NASA
%Origin             CDS
%Id                 P/allWISE/W4
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allwise/expsup/sec1_6b.html
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%Aladin.Tree        Image/Infrared/WISE
%Aladin.MenuNumber  04-003-04
%Aladin.HpxParam    8 image equatorial jpeg fits
%Aladin.Date        2016-06-03T14:58Z

%ActionName         P-allWISE-color.hpx
%Description        AllWISE color  Red (W4) , Green (W2) , Blue (W1) from raw Atlas Images
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%SeeAction          P-allWISE-color_0.hpx availability=0
%SeeAction          P-allWISE-color_1.hpx availability=9999
%SeeAction          P-allWISE-color_2.hpx availability=9999
%SeeAction          P-allWISE-color_3.hpx availability=9999
%SeeAction          P-allWISE-color_4.hpx availability=9999
%SeeAction          P-allWISE-color_5.hpx availability=1055
%SeeAction          P-allWISE-color_6.hpx availability=9999
%VerboseDescr       NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5\u03c3 point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background. The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.
%Copyright          IPAC/NASA
%Origin             CDS
%Id                 P/allWISE/color
%Aladin.Profile     >6.1
%Copyright.Url      http://wise2.ipac.caltech.edu/docs/release/allsky/
%SkyFraction        1
%Aladin.XLabel      The Wide-field Infrared Survey Explorer - W4-W2-W1 bands (allWISE color RGB-W4-W2-W1)
%Aladin.Tree        Image/Infrared/WISE
%Aladin.MenuNumber  04-003-00 lite
%Aladin.HpxParam    8 image color equatorial jpeg
%Aladin.Date        2016-07-01T06:44Z

%ActionName         P-bice.hpx
%Description        ID1490928593
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://darts.isas.jaxa.jp/pub/judo2/HiPS/bice
%Origin             JAXA
%Id                 P/bice
%Aladin.Profile     >6.1
%SkyFraction        0.02512
%Aladin.XLabel      ID1490928593
%Aladin.HpxParam    3 image color equatorial png fits
%Aladin.Date        2017-03-31T02:50Z

%ActionName         P-cda-hips-allsky-rgb.hpx
%Description        CXC HiPS
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1563821297  2019/07/22 20:48:17
%Url                https://cdaftp.cfa.harvard.edu/cxc-hips
%VerboseDescr       CXC public observations as of 2018/03/01
%Copyright          Chandra Data Archive (http://cxc.cfa.harvard.edu/cda/)
%Origin             cxc.harvard.edu
%Id                 P/cda/hips/allsky/rgb
%Aladin.Profile     >6.1
%SkyFraction        0.02191
%Aladin.XLabel      CDA
%Aladin.Tree        Image/X/CXC
%Aladin.HpxParam    11 image color live equatorial png
%Aladin.Date        2019-06-17T15:22Z

%ActionName         P-omega-albedo_filled.hpx
%Description        omega albedo_filled
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_albedo_filled
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/albedo_filled
%Aladin.Profile     >6.1 beta
%SkyFraction        1
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-01T15:12Z

%ActionName         P-omega-albedo_r1080.hpx
%Description        omega albedo_r1080
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_albedo_r1080
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/albedo_r1080
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9854
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T14:40Z

%ActionName         P-omega-albedo_unfilled.hpx
%Description        omega albedo_unfilled
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_albedo_unfilled
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/albedo_unfilled
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9771
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-01T16:01Z

%ActionName         P-omega-emissivite_5-03mic.hpx
%Description        omega emissivite_5-03mic
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_emissivite_5-03mic
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/emissivite_5-03mic
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9942
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T13:55Z

%ActionName         P-omega-emissivite_5-05mic.hpx
%Description        omega emissivite_5-05mic
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_emissivite_5-05mic
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/emissivite_5-05mic
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9942
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T13:58Z

%ActionName         P-omega-emissivite_5-07mic.hpx
%Description        omega emissivite_5-07mic
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_emissivite_5-07mic
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/emissivite_5-07mic
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9942
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T13:59Z

%ActionName         P-omega-emissivite_5-09mic.hpx
%Description        omega emissivite_5-09mic
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_emissivite_5-09mic
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/emissivite_5-09mic
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9942
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T14:05Z

%ActionName         P-omega-ferric_bd530.hpx
%Description        omega ferric_bd530
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_ferric_bd530
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/ferric_bd530
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9283
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-10-17T14:42Z

%ActionName         P-omega-ferric_nnphs.hpx
%Description        omega ferric_nnphs
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_ferric_nnphs
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/ferric_nnphs
%Aladin.Profile     >6.1 beta
%SkyFraction        0.9285
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-09-17T14:28Z

%ActionName         P-omega-olivine_osp1.hpx
%Description        omega olivine_osp1
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_olivine_osp1
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/olivine_osp1
%Aladin.Profile     >6.1 beta
%SkyFraction        0.02673
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-09-17T14:29Z

%ActionName         P-omega-olivine_osp2.hpx
%Description        omega olivine_osp2
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_olivine_osp2
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/olivine_osp2
%Aladin.Profile     >6.1 beta
%SkyFraction        0.002061
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-09-17T14:29Z

%ActionName         P-omega-olivine_osp3.hpx
%Description        omega olivine_osp3
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_olivine_osp3
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/olivine_osp3
%Aladin.Profile     >6.1 beta
%SkyFraction        0.002444
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-09-17T14:29Z

%ActionName         P-omega-pyroxene_bd2000.hpx
%Description        omega pyroxene_bd2000
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://healpix.ias.u-psud.fr/idoc_P_omega_pyroxene_bd2000
%VerboseDescr       Omega Mineral maps are OMEGA-base maps. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003.
%Origin             idoc
%Id                 P/omega/pyroxene_bd2000
%Aladin.Profile     >6.1 beta
%SkyFraction        0.5203
%Aladin.XLabel      Omega mineral maps - Mars Express
%Aladin.Tree        Solar system/Mars/Omega
%Aladin.HpxParam    3 image mars png fits
%Aladin.Date        2018-09-17T14:35Z

%ActionName         P-skymapper-G.hpx
%Description        Skymapper G-band
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_G
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-G
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%ActionName         P-skymapper-I.hpx
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%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_I
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-I
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%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
%SkyFraction        0.4917
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%Aladin.Date        2017-09-24T17:14Z

%ActionName         P-skymapper-R.hpx
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%Owner              CDS'aladin
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%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_R
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-R
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%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
%SkyFraction        0.5
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%Aladin.HpxParam    9 image equatorial png fits
%Aladin.Date        2017-09-28T06:53Z

%ActionName         P-skymapper-U.hpx
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%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_U
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-U
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%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
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%Aladin.HpxParam    9 image equatorial png fits
%Aladin.Date        2017-10-25T18:21Z

%ActionName         P-skymapper-V.hpx
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%Owner              CDS'aladin
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%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_V
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
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%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
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%ActionName         P-skymapper-Z.hpx
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%VersionNumber      1551076531  2019/02/25 08:35:31
%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_Z
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98% of the southern sky, mostly covering the range from the South Celestial Pole to +2 deg in declination, with some extra coverage reaching +10 deg. Included are fields observed between March 2014 and September 2015, with a number of quality cuts applied. Each visit to a given field includes an exposure in all six filters, uvgriz, although on some fields (12%) not all filter images passed the quality cuts. Measurements from over 2.3 billion detections covering over 20,200 deg2 of sky are available. HiPS made by CDS from the original images (sky background removed by SKymapper team).
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-Z
%Aladin.Profile     >6.1
%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
%SkyFraction        0.496
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%Aladin.Tree        Image/Optical/Skymapper
%Aladin.MenuNumber  03-xx
%Aladin.HpxParam    9 image equatorial png fits
%Aladin.Date        2017-11-12T22:20Z

%ActionName         P-skymapper-color.hpx
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%Url                http://alasky.u-strasbg.fr/Skymapper/skymapper_color
%VerboseDescr       The SkyMapper First Data Release provides data from the Shallow Survey across >98%
%Copyright          Australian National University
%Origin             CDS
%Id                 P/skymapper-color
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%Copyright.Url      http://skymapper.anu.edu.au/policies/authorship/
%SkyFraction        0.508
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%Aladin.Date        2017-11-20T06:46Z

%ActionName         PASP.fullpaper
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%Owner              CDS'extern
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%ActionName         Portal.logo
%Description        Icone pour le portail
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1287144134  2010/10/15 14:02:14
%Url                http://cdsportal.u-strasbg.fr
%FullTextResult     <a href="$url"><img src="http://cdsarc.u-strasbg.fr/CDS/cdsportal_icon.gif" alt="Portal icon" border="0" /></a>

%ActionName         Portal.sesameService
%Description        Service Sesame (JSON ou XML) en backend du portail
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1481831838  2016/12/15 21:57:18
%Url                http://cdsportal.u-strasbg.fr/services/sesame?object=$1&format=$2
%Test               param="M1 json" pattern="83.63"

%ActionName         QUB.home
%Description        Queen's University Belfast, School of Computer Science
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1  2001/12/31 15:08:19
%Url                http://www.qub.ac.uk/
%DefaultAnchorText  QUB

%ActionName         Qualifier
%Description        Get the qualifiers for a position from the Aladin image server
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://aladin.cds.unistra.fr/AladinPreview?-c=$1&out=qualifier

%ActionName         Qualifier-test
%Description        Get the qualifiers for a position from the Aladin image server
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1490859993  2017/03/30 09:46:33
%Url                http://aladix.u-strasbg.fr/java/alapre-test.pl?-c=$1&out=qualifier

%ActionName         Qualifier.GOODS
%Description        Get the qualifiers for a position from the New Aladin image server
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1490859993  2017/03/30 09:46:33
%Url                http://aladix.u-strasbg.fr/cgi-bin/nph-HTTP1.cgi?out=qualifier&position=$1&radius=$2

%ActionName         QueryCat.test
%Description        Test de QueryCat
%Owner              CDS'querycat
%DistribDomain      CDS
%VersionNumber      1340700229  2012/06/26 10:43:49
%Url                http://cdsxmatch.u-strasbg.fr/QueryCat/QueryCat?catName=$1&mode=cone&pos=$2&r=$3arcmin&format=csv&limit=3
%Param.Description  $1=Catalog name
%Param.Description  $2=Target
%Param.Description  $3=Radius
%Param.DataType     $1=E
%Param.DataType     $2=J2000
%Test               param="SDSS8 240.36647+29.84967 10" pattern="240"
%ResultDataType     Mime(text/csv)

%ActionName         QueryCatDaemon
%Description        QueryCatDaemon for VizieR
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1578055402  2020/01/03 14:43:22
%SeeAction          QueryCatDaemon.axel availability=1
%SeeAction          QueryCatDaemon.iucaa availability=2

%ActionName         QueryCatDaemon.ch
%Description        Big catalogue server (FX) (in china)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1720172344  2024/07/05 11:39:04
%Url                http://vizier.china-vo.org/viz-bin/qat2s_asu.cgi?--source=$1&--c=$2&--out.max=$3&--c.rm=1&--host=vizier.china-vo.org
%Test               param="wise_allsky 0+0 1" pattern="WISE"

%ActionName         QueryCatDaemon.vizier
%Description        Big catalogue server (FX) (on vizier)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1720167763  2024/07/05 10:22:43
%Url                https://vizier.cds.unistra.fr/viz-bin/qat2s_asu.cgi?--source=$1&--c=$2&--out.max=$3&--c.rm=2&--host=vizcat.cds.unistra.fr
%Test               param="2mass6x 89.9-67.5 1" pattern="2MASS6X"

%ActionName         Question Feedback
%Description        Anchor for cds-question@unistra.fr
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1531208993  2018/07/10 09:49:53
%Url                mailto:cds-question@unistra.fr?Subject=$1
%FullTextResult     Please send comments and questions to <A HREF="$url">\ncds-question@unistra.fr</A>

%ActionName         RDAEurope.home
%Description        Home page du projet RDA Europe
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1372073572  2013/06/24 13:32:52
%Url                http://europe.rd-alliance.org/

%ActionName         SDSS-DR12.cat
%Description        SLOAN SDSS DR12 catalog
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                http://skyserver.sdss.org/dr12/en/tools/search/x_results.aspx?searchtool=Radial&coordtype=equatorial&ra=$1&dec=$2&radius=$3&format=votable&limit=0
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius (arcmin)
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUS)
%ResultDataType     Mime(text/xml)
%Doc.User           http://skyserver.sdss.org/dr12/en/tools/search/radial.aspx
%Aladin.Profile     <10.144
%Aladin.Label       SLOAN SDSS DR12
%Aladin.Menu        Others..
%Aladin.LabelPlane  SDSS DR12 $1 $2 $3

%ActionName         SDSS-lastDR
%Description        SDSS images (last release)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576256031  2019/12/13 18:53:51
%Url                http://skyserver.sdss.org/vo/SIAP/SIAP.asmx/getSiapInfo?POS=$1,$2&SIZE=$3&FORMAT=image/fits&BANDPASS=ugriz
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.Value        $3=0.17
%ResultDataType     Mime(sia/xml)
%Aladin.Label       SDSS
%Aladin.LabelPlane  SDSS
%Aladin.Logo        SDSSLogo.gif

%ActionName         SDSS.drX.id
%Description        Get details of last SDSS-IV (release XXX) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1692795605  2023/08/23 15:00:05
%Url                http://skyserver.sdss.org/dr$1/en/tools/explore/summary.aspx?id=$2
%Param.Description  $1=DR version number
%Param.Description  $2=SDSS-Identification (18-digit number)
%Param.Value        $2=17
%Param.Value        $2=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS.drX.pos
%Description        Get details of last SDSS-IV (release XXX) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1692795605  2023/08/23 15:00:05
%Url                http://skyserver.sdss.org/dr$1/en/tools/explore/summary.aspx?ra=$2&dec=$3
%Param.Description  $1=DR version number
%Param.Description  $2=Right ascension (J2000)
%Param.Description  $3=Declination (J2000), decimal degrees
%Param.DataType     $2=Coo(J2000,RAdeg)
%Param.DataType     $3=Coo(J2000,DEdeg)
%Param.Value        $1=17
%Param.Value        $2=0
%Param.Value        $3=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS.drX.sp3
%Description        Interactive spectrum from SDSS-IV (release XXX) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1692795605  2023/08/23 15:00:05
%Url                http://skyserver.sdss.org/dr$1/en/tools/explore/summary.aspx?plate=$2&mjd=$3&fiber=$4
%Param.Description  $1=DR version number
%Param.Description  $2=Plate number
%Param.Description  $3=MJD of observation
%Param.Description  $4=Filber number
%Param.Value        $1=17
%Param.Value        $2=1489
%Param.Value        $3=52991
%Param.Value        $4=180
%ResultDataType     Mime(text/html)

%ActionName         SDSS.id
%Description        Get details of last SDSS release from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1692795605  2023/08/23 15:00:05
%Url                http://cas.sdss.org/astro/en/tools/explore/obj.asp?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=587726032791995128
%ResultDataType     Mime(text/html)

%ActionName         SDSS.pos
%Description        Get details of SDSS7 release from ra,dec
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/tools/explore/obj.asp?ra=$1&dec=$2
%Param.Description  $1=Right Ascension (J2000), decimal degrees
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=195.001179
%Param.Value        $2=2.504048
%ResultDataType     Mime(text/html)

%ActionName         SDSS.query
%Description        Get a result of a SQL query on SDSS7 release (html)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/tools/search/x_sql.asp?cmd=$1&format=html
%Param.Description  $1=SQL Query
%Param.Value        $1=Select * from PhotoObjAll where objID=587726032791995128
%ResultDataType     Mime(text/html)

%ActionName         SDSS.sp
%Description        Get details of spectroscopic target from SDSS7 release from spID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/get/specById.asp?id=$1
%Param.Description  $1=SDSS-Spectro-Identification (18-digit number)
%Param.Value        $1=79597814924967936
%ResultDataType     Mime(text/html)

%ActionName         SDSS.sp3
%Description        Get details of SDSS7 release from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/tools/explore/obj.asp?plate=$1&mjd=$2&fiber=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1050
%Param.Value        $2=52721
%Param.Value        $3=402
%ResultDataType     Mime(text/html)

%ActionName         SDSS.sp3.fits
%Description        Get FITS spectrum from SDSS (release<=7) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/tools/explore/obj.asp?plate=$1&mjd=$2&fiber=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation (>50000)
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=489
%ResultDataType     Mime(text/html)

%ActionName         SDSS.sql
%Description        Get a result of a SQL query on SDSS7 release as comma-separated-values
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cas.sdss.org/astro/en/tools/search/x_sql.asp?cmd=$1&format=csv
%Param.Description  $1=SQL Query
%Param.Value        $1=Select * from PhotoObjAll where objID=587726032791995128
%ResultDataType     Mime(application/text)

%ActionName         SDSS3.dr12.id
%Description        Get details of last SDSS-III (release 12) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss3.org/dr12/en/tools/explore/summary.aspx?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.dr12.pos
%Description        Get details of last SDSS-III (release 12) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss3.org/dr12/en/tools/explore/summary.aspx?ra=$1&dec=$2
%Param.Description  $1=Right ascension (J2000)
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=0
%Param.Value        $2=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.dr12.sp3
%Description        Interactive spectrum from SDSS-III (release 12) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://dr12.sdss.org/spectrumDetail?plateid=$1&mjd=$2&fiber=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=180
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.id
%Description        Get details of last SDSS-III (release>=8) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss3.org/dr9/en/tools/quicklook/quickobj.asp?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.pos
%Description        Get details of target from SDSS-III (release>=8) from RA+Dec
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss3.org/dr9/en/tools/quicklook/quickobj.asp?ra=$1&dec=$2
%Param.Description  $1=Right Ascension (J2000), decimal degrees
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=359.836494
%Param.Value        $2=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.sp
%Description        Get details of spectroscopic target from SDSS-III (release>=8) from spID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss3.org/dr9/en/get/specById.asp?id=$1
%Param.Description  $1=SDSS-Spectro-Identification (18-digit number)
%Param.Value        $1=435776895187970048
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.sp3
%Description        Interactive spectrum from SDSS-III (release>=8) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://dr9.sdss3.org/spectrumDetail?plateid=$1&mjd=$2&fiber=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=180
%ResultDataType     Mime(text/html)

%ActionName         SDSS3.sp3.fits
%Description        Get FITS spectrum from SDSS-III (release>=8) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://dr9.sdss3.org/dr9-cgi/getSpectra/fits?plate=$1&mjd=$2&fiber=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation (>50000)
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=489
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr14.id
%Description        Get details of last SDSS-IV (release 14) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss.org/dr14/en/tools/explore/summary.aspx?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr14.pos
%Description        Get details of last SDSS-IV (release 14) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://skyserver.sdss.org/dr14/en/tools/explore/summary.aspx?ra=$1&dec=$2
%Param.Description  $1=Right ascension (J2000)
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=0
%Param.Value        $2=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr14.sp3
%Description        Interactive spectrum from SDSS-IV (release 14) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://dr14.sdss.org/optical/spectrum/view?plateid=$1&mjd=$2&fiberid=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=180
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr15.id
%Description        Get details of last SDSS-IV (release 15) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://skyserver.sdss.org/dr15/en/tools/explore/summary.aspx?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr15.pos
%Description        Get details of last SDSS-IV (release 15) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://skyserver.sdss.org/dr15/en/tools/explore/summary.aspx?ra=$1&dec=$2
%Param.Description  $1=Right ascension (J2000)
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=0
%Param.Value        $2=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr15.sp3
%Description        Interactive spectrum from SDSS-IV (release 15) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://dr15.sdss.org/optical/spectrum/view?plateid=$1&mjd=$2&fiberid=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=180
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr16.id
%Description        Get details of last SDSS-IV (release 16) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://skyserver.sdss.org/dr16/en/tools/explore/summary.aspx?id=$1
%Param.Description  $1=SDSS-Identification (18-digit number)
%Param.Value        $1=1237657190905086089
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr16.pos
%Description        Get details of last SDSS-IV (release 16) from objID
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://skyserver.sdss.org/dr16/en/tools/explore/summary.aspx?ra=$1&dec=$2
%Param.Description  $1=Right ascension (J2000)
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=0
%Param.Value        $2=-0.279038
%ResultDataType     Mime(text/html)

%ActionName         SDSS4.dr16.sp3
%Description        Interactive spectrum from SDSS-IV (release 16) from plate-MJD-fiber
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1593087357  2020/06/25 14:15:57
%Url                http://dr16.sdss.org/optical/spectrum/view?plateid=$1&mjd=$2&fiberid=$3
%Param.Description  $1=Plate number
%Param.Description  $2=MJD of observation
%Param.Description  $3=Filber number
%Param.Value        $1=1489
%Param.Value        $2=52991
%Param.Value        $3=180
%ResultDataType     Mime(text/html)

%ActionName         SED
%Description        VizieR SED generator
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1354611371  2012/12/04 10:56:11
%SeeAction          VizieR.sed availability=10000
%Param.Description  $1=Object or coordinates
%Param.Description  $2=Radius (arcsec)
%Param.DataType     $1=Target(COO)
%Param.Value        $2=5
%ResultDataType     Mime(application/xml)
%VerboseDescr       This form is dedicated to query VizieR Spectral Energy Distribution (SED) builder. The result is a table of various photometry points (Jansky vs Frequence) computed by VizieR from a list of photometry catalogs. Select the plane in the Aladin stack for drawing the SED.
%Aladin.Menu        Tools...
%Aladin.Label       VizieR SED
%Aladin.labelPlane  SED $1
%Aladin.Profile     >7.536

%ActionName         SF.fits
%Description        Get Full FITS Extract from SIRTF
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.cv.nrao.edu/cgi-bin/SFpostage.pl?Equinox=J2000&RA=$1&Dec=$2&Size=$3+$3&Cells=1.0+1.0&MAPROJ=SIN&Type=image/x-fits
%Param.Description  $1=Right ascension (J2000)
%Param.Description  $2=Declination (J2000)
%Param.Description  $3=Dimension in arcmin
%Param.Value        $3=5.0
%ResultDataType     Mime(image/fits)

%ActionName         SIA
%Description        Generic SIAv1 query
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1507562904  2017/10/09 17:28:24
%Url                $4POS=$1,$2&SIZE=$3&FORMAT=image/fits
%Param.Description  $4=Base URL (incl. '?')
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.DataType     $4=BaseUrl
%Param.Value        $3=0.17
%ResultDataType     Mime(text/xml)
%Aladin.Menu        VO protocols..
%Aladin.XLabel      Generic Simple Image Access v1 query
%Aladin.LabelPlane  $4
%Aladin.Profile     >10

%ActionName         SIA2
%Description        Generic SIAv2 query
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1508724361  2017/10/23 04:06:01
%Url                $4POS=CIRCLE+$1+$2+$3&ID=$5&COLLECTION=$6&FACILITY=$7&INSTRUMENT=$8&TARGET=$9&CALIB=$10&MAXREC=$11
%Param.Description  $4=Server IVOID or base URL
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.Description  $5=Data set identifier
%Param.Description  $6=Collection name
%Param.Description  $7=Telescope name
%Param.Description  $8=Instrument name
%Param.Description  $9=Target
%Param.Description  $10=Calibration level (0..3)
%Param.Description  $11=Maximum number of rec
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.DataType     $4=BaseUrl(URL|ID)
%Param.Value        $3=0.17
%Param.Value        $11=99999
%Param.Value        $11=9999
%Param.Value        $11=999
%Param.Value        $11=99
%ResultDataType     Mime(text/xml)
%Aladin.Menu        VO protocols..
%Aladin.XLabel      Generic Simple Image Access v2 query
%Aladin.LabelPlane  $4
%Aladin.Profile     >10

%ActionName         SIMBAD.logo.mini
%Description        SIMBAD logo
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1277298706  2010/06/23 15:11:46
%FullTextResult     <IMG SRC="<&CDSheadU>simbad_70x35.png" ALT="Simbad">
%ResultDataType     Mime(image/png)

%ActionName         SIMBAD4
%Description        Description of SIMBAD4
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1470738217  2016/08/09 12:23:37
%Url                <&SimbadHelp>=simbad4
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SIMBADQUERYCOOFORM
%Description        Simbad query coordinate form
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1189409429  2007/09/10 09:30:29
%Url                <&SimbadUrl>/sim-fcoo?coord=$1
%FullTextResult     <A HREF="$url" target="_top">$text</A>
%Param.Description  $1=coordinates
%Param.Optional     $1
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SIMBADQUERYIDFORM
%Description        Simbad query id form
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1189409429  2007/09/10 09:30:29
%Url                <&SimbadUrl>/sim-fid
%FullTextResult     <A HREF="$url" target="_top">$text</A>
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SIMBADQUERYREFFORM
%Description        Simbad query reference form
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1189409429  2007/09/10 09:30:29
%Url                <&SimbadUrl>/sim-fref?bibcode=$1
%FullTextResult     <A HREF="$url" target="_top">$text</A>
%Param.Description  $1=bibcode
%Param.DataType     $1=B
%Param.Optional     $1
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SIMBADSAMPLEFORM SIMBADQUERYSAMPLEFORM
%Description        Simbad sample form
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-fsam
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SIMBADSCRIPTFORM SIMBADQUERYLISTFORM
%Description        Simbad sample query form.
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-fscript
%Test               noparam
%ResultDataType     Mime(text/html)

%ActionName         SMB.O simbo
%Description        Simbad query by a bibliographical reference for the object list
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1229092752  2008/12/12 16:39:12
%Url                <&SimbadUrl>/sim-ref?bibcode=$1&simbo=on&submit=submit%20bibcode
%Param.Description  $1=Bibcode
%Param.DataType     $1=B
%Test               param="1995A&AS..111...41N"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SPLAT
%Description        Spectral Analysis Tool
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1634044739  2021/10/12 15:18:59
%VerboseDescr       SPLAT is a graphical tool for displaying, comparing, modifying and analysing astronomical spectra stored in NDF, FITS and TEXT files as well as the new NDX format. It can read spectra from local disk files, download them over the Internet, or it can interact with the Virtual Observatory and query servers for spectral data in a region of the sky.
%Institute          PPARC, supported by JAC (Hawaii)
%Copyright          SPLAT is available under the terms of the GNU General Public License
%Doc.User           http://star-www.dur.ac.uk/~pdraper/splat/splat-vo
%ReleaseNumber      3.9.0 (SAMP compatible)
%Webstart           http://star-www.dur.ac.uk/~pdraper/starjava/splat.jnlp
%Aladin.Activated   No
%Aladin.VOLabel     SPLAT spectral analysis tool [Starlink/PPARC/JAC]

%ActionName         SSA
%Description        Generic SSA v1 query
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1507562904  2017/10/09 17:28:24
%Url                $4POS=$1,$2&SIZE=$3&REQUEST=queryData
%Param.Description  $4=Base URL (incl. '?')
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.DataType     $4=BaseUrl
%Param.Value        $3=0.17
%ResultDataType     Mime(text/xml)
%Aladin.Menu        VO protocols..
%Aladin.XLabel      Generic Simple Spectra Access query
%Aladin.LabelPlane  $4
%Aladin.Profile     >10

%ActionName         SSS.Ha
%Description        Get Images of SuperCosmos Ha-Survey (FITS)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www-wfau.roe.ac.uk/~sss/cgi-bin/hapixel.cgi/cgi-bin/hapixel.cgi?coords=$1&equinox=2&size=$2&sizey=$2&waveband=$3&output=4&gif=0
%Param.Description  $1=Coordinates HH MM SS.S +DD MM SS (J2000)
%Param.Description  $2=Size of box in arcmin
%Param.Description  $3=Survey: 1=Halpha, 2=ShortRed, 3=Both
%Param.Value        $1=17 34 59.10 -56 49 24.0
%Param.Value        $2=4
%Param.Value        $3=1
%ResultDataType     Mime(text/html)

%ActionName         SSS.cat
%Description        SuperCOSMOS catalog server - Edinburgh (UK)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                http://www-wfau.roe.ac.uk/~sss/cgi-bin/sss_aladin_obj.cgi?ra=$1&dec=$2&xsize=$3&ysize=$4&waveband=$5
%Param.Description  $1=Right Ascension (J2000)
%Param.Description  $2=Declination (J2000)
%Param.Description  $3=Width (arcmin)
%Param.Description  $4=Height (arcmin)
%Param.Description  $5=Waveband
%Param.DataType     $1=Target(RA)
%Param.DataType     $2=Target(DE)
%Param.DataType     $3=Field(RA)
%Param.DataType     $4=Field(DE)
%Param.Value        $3=10
%Param.Value        $4=10
%Param.Value        $5=1 - UKST Blue (Bj)
%Param.Value        $5=2 - UKST Red (R)
%Param.Value        $5=3 - UKST Infrared (I)
%Param.Value        $5=4 - ESO red (R)
%Param.Value        $5=5 - POSS-I red (R)
%ResultDataType     Mime(text/xml)
%Doc.User           http://www-wfau.roe.ac.uk/sss/
%Aladin.Label       SuperCOSMOS catalog (SSS.cat)
%Aladin.Menu        Others..
%Aladin.Profile     <10.144
%Aladin.LabelPlane  SSS $5

%ActionName         SSS.img
%Description        SuperCOSMOS image server- Edinburgh (UK)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                http://www-wfau.roe.ac.uk/~sss/cgi-bin/sss_aladin_pix.cgi?ra=$1&dec=$2&mime-type=image/x-gfits&x=$3&y=$4&waveband=$5
%Param.Description  $1=Right Ascension (J2000)
%Param.Description  $2=Declination (J2000)
%Param.Description  $3=Width (arcmin)
%Param.Description  $4=Height (arcmin)
%Param.Description  $5=Waveband
%Param.DataType     $1=Target(RA)
%Param.DataType     $2=Target(DE)
%Param.DataType     $3=Field(RA)
%Param.DataType     $4=Field(DE)
%Param.Value        $3=10
%Param.Value        $4=10
%Param.Value        $5=1 - UKST Blue (Bj)
%Param.Value        $5=2 - UKST Red (R)
%Param.Value        $5=3 - UKST Infrared (I)
%Param.Value        $5=4 - ESO red (R)
%Param.Value        $5=5 - POSS-I red (R)
%ResultDataType     Mime(image/gfits)
%Doc.User           http://www-wfau.roe.ac.uk/sss/
%Aladin.Label       SuperCOSMOS images  (SSS.img)
%Aladin.Menu        Others...
%Aladin.Profile     <10.144
%Aladin.LabelPlane  SSS $5

%ActionName         STECF.home
%Description        Space Telescope - European Coordinating Facility
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      2  2001/11/21 10:54:33
%Url                http://www.stecf.org/
%DefaultAnchorText  ST-ECF

%ActionName            SUBARU_Suprime-Cam
%Description           Subaru Suprime-Cam
%Owner              CDS'aladin
%DistribDomain         ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                   http://jvo.nao.ac.jp/skynode/do/siap/spcam/image_cutout/1.0?FORMAT=image/fits&POS=$1,$2&SIZE=$3,$4
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Width (deg)
%Param.Description  $4=Height (deg)
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RAd)
%Param.DataType     $4=Field(DEd)
%Param.Value        $3=0.17
%Param.Value        $4=0.17
%ResultDataType        Mime(sia/xml)
%VerboseDescr        Allows access (via SIAP) to Subaru Suprime-Cam images (The Subaru Prime Focus Camera (Suprime-Cam) is a mosaic of ten 2048 x 4096 CCDs, located at the prime focus of Subaru Telescope, which covers a 34' x 27' field of view with a pixel scale of 0.20'').
%Institute           Japan Virtual Observatory
%Doc.User            http://subarutelescope.org/Observing/Instruments/SCam/index.html
%Aladin.Profile     <10.144
%Aladin.Menu        Archives...
%Aladin.Label       Subaru Suprime-Cam
%Aladin.LabelPlane  Suprime

%ActionName         SUMSS.fits
%Description        Get FITS Mosaic from SUMSS
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.astrop.physics.usyd.edu.au/mosaics/$1/$2.FITS
%Param.Description  $1=Galactic or Extragalactic
%Param.Description  $2=File Name
%ResultDataType     Mime(image/fits)

%ActionName         Script.Tutorial
%Description        The full CDS Tutorial
%Owner              CDS'glu
%DistribDomain      CDS
%VersionNumber      1350312443  2012/10/15 16:47:23
%Url                <&CDS.Tutorial,u>
%ResultDataType     Mime(text/html)

%ActionName         Sesame
%Description        CDS Sesame resolver
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1679318975  2023/03/20 15:29:35
%Url                http://cds.unistra.fr/cgi-bin/nph-sesame/-oI/SVN?$1
%Test               param="M1" pattern="05.34.*22.0"

%ActionName         Sesame.Service
%Description        CDS resolver (target name to coordinates)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://cds.unistra.fr/cgi-bin/Sesame?$1
%FullTextResult     <a href='https://cds.unistra.fr/cgi-bin/Sesame?$1'>Sesame</a>
%Param.DataType     $1=I
%Test               param="V1357 Cyg" pattern="HD 226868"
%ResultDataType     Mime(text/plain)
%Doc.User           https://cds.unistra.fr/doc/sesame.htx

%ActionName         Sesame.WS
%Description        Object name resolver by Web Services
%Owner              CDS'ws
%DistribDomain      CDS
%VersionNumber      1373967572  2013/07/16 11:39:32
%SeeAction          Sesame.WS.fr availability=0
%SeeAction          Sesame.WS.us availability=1055
%SeeAction          Sesame.WS.ca availability=1055
%SeeAction          Sesame.WS.jp availability=9999

%ActionName         Sesame.WS.fr.bis
%Description        Object name resolver by Web services (CDS - Strasbourg) - backup
%Owner              CDS'ws
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cdsws2.u-strasbg.fr/axis/services/Sesame?$1
%Test               param="method=sesame&name=hd226868" option="n" pattern="=Simbad"
%Test               param="wsdl" pattern="SesameResponse"
%ResultDataType     soap
%Doc.Technical      http://cds.unistra.fr/cdsws/name_resolver.gml

%ActionName         Sesame.jsonp
%Description        Service Sesame retournant du JSONP [utilisé par Aladin Lite]
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1677663158  2023/03/01 11:32:38
%Url                http://cds.unistra.fr/cgi-bin/nph-sesame.jsonp?object=$1&callback=$2
%Test               param="hd42195 myCallback" pattern="92.8"

%ActionName         SimViz
%Description        Details for a SIMBAD Identification
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/viz-bin/VizieR-S?$1
%Param.DataType     $1=I
%Test               param="\"V* R AND\""
%Test               param="\"HIP 12345\""
%ResultDataType     Mime(text/html)

%ActionName         Simbad.Tutorial
%Description        Simbad tutorial
%Owner              CDS'glu
%DistribDomain      CDS
%VersionNumber      1350312443  2012/10/15 16:47:23
%FullTextResult     <&CDS.Tutorial,u>#simbadTutorial
%ResultDataType     Mime(text/html)

%ActionName         Simbad.logo
%Description        Simbad logo.
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1268472392  2010/03/13 11:26:32
%SeeAction          Simbad.logo.viz availability=9999
%SeeAction          Simbad.logo.rel availability=9999
%SeeAction          Simbad.logo.abs availability=6

%ActionName         Simbad.logo.tiny
%Description        Aladin logo
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&CDSheadU>/simbad_35x18.png
%FullTextResult     <IMG SRC="$url" alt="simbad">
%ResultDataType     Mime(image/png)
%DefaultAction      simbad

%ActionName         SimbadD.us
%Description        Simbad display mirror prefix (USA)
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1721738169  2024/07/23 14:36:09
%FullTextResult     http://simbad.harvard.edu/simbad/sim-display?data

%ActionName         SimbadDisplay
%Description        Simbad Display documentation
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1722948168  2024/08/06 14:42:48
%SeeAction          SimbadD.fr availability=1

%ActionName         SimbadG.us
%Description        Simbad guide mirror prefix (USA)
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1721738064  2024/07/23 14:34:24
%FullTextResult     http://simbad.harvard.edu/guide

%ActionName         SimbadGlobal
%Description        Test global de Simbad
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1362059067  2013/02/28 15:44:27
%Url                <&SimbadUrl,u>/sim-id?Ident=$1
%Test               param="HD1" pattern="K0"

%ActionName         SimbadGuide
%Description        Simbad guide documentation
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1722948168  2024/08/06 14:42:48
%SeeAction          SimbadG.fr availability=-1

%ActionName         SimbadH.us
%Description        Simbad help mirror prefix (USA)
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1721738064  2024/07/23 14:34:24
%FullTextResult     http://simbad.harvard.edu/simbad/sim-help?Page

%ActionName         SimbadHelp
%Description        Simbad generic Help
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1721738169  2024/07/23 14:36:09
%SeeAction          SimbadH.fr availability=1

%ActionName         SimbadIntro
%Description        What is SIMBAD, and what is not ?
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1470738217  2016/08/09 12:23:37
%Url                <&SimbadUrl>/guide/SimbadIntro.htx
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         SimbadQuick
%Description        Simbad finger facility (return object with the largest biblio ref)
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1698066819  2023/10/23 15:13:39
%Url                https://simbad.cds.unistra.fr/cone-aladin/?RADEC=$1&SR=$2&RESPONSEFORMAT=aladin
%Test               param="00+05+08.48+%2B67+50+26.1 0.015" option="n" pattern="HD *1"

%ActionName         SimbadResolve
%Description        Simbad resolver (target name to coordinates)
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1  2001/12/10 14:35:23
%Url                <&SimbadU>/simbad-getcoord.pl?Ident=$1

%ActionName         SimbadU
%Description        Simbad mirror site management
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1127725585  2005/09/26 10:06:25
%SeeAction          SimbadU.fr availability=9999
%SeeAction          SimbadU.us availability=9999

%ActionName         SimbadUrl
%Description        Simbad url root path
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1359724820  2013/02/01 15:20:20
%SeeAction          SimbadUrl.fr availability=8
%SeeAction          SimbadUrl.us availability=9999

%ActionName         SimbadXML
%Description        Query Simbad to retrieve object list around a target in XML format
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/cgi/simbad-flat/simbad-cs.py?target=$1&SR=$2&format=votable-tsv&SRUNIT=arcmin&SORTBY=nbref
%Test               param="'18 55 03.28 -30 28 42.6' 14" pattern="HD 174952"

%ActionName         Simplay
%Description        Simplay (Flash Simbad viewer)
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/SimPlay
%Test               noparam pattern="simplay"
%ResultType         Mime(text/html)

%ActionName         SimplayTest
%Description        Test du CGI utilisé par SimPlay
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1677663158  2023/03/01 11:32:38
%Url                http://alasky.cds.unistra.fr/cgi/simplay/simplay-simbad.py?mode=getLinks&target=$1&imsize=$2&imtype=$3
%Test               param="NGC7331 14 color" pattern="skycoord"

%ActionName         SkyBoT.IMCCE
%Description        Solar system object database from IMCCE
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1433488019  2015/06/05 09:06:59
%Url                http://vo.imcce.fr/webservices/skybot/skybotconesearch_query.php?-ep=$1&-ra=$2&-dec=$3&-size=$4,$5&-mime=votable&-out=basic&-loc=$6&-search=$7&-filter=$8&-from=Aladin
%Param.Description  $1=Epoch
%Param.Description  $2=Right Ascension
%Param.Description  $3=Declination
%Param.Description  $4=Width (arcmin)
%Param.Description  $5=Height (arcmin)
%Param.Description  $6=Observer location
%Param.Description  $7=Search for
%Param.Description  $8=Max. uncertainty
%Param.DataType     $1=Date(JD)
%Param.DataType     $2=Target(RAd)
%Param.DataType     $3=Target(DEd)
%Param.DataType     $4=Field(RA)
%Param.DataType     $5=Field(DE)
%Param.Value        $6=500
%Param.Value        $7=Asteroids and Planets
%Param.Value        $7=Asteroids, Planets and Comets
%Param.Value        $7=Asteroids and Comets
%Param.Value        $7=Planets and Comets
%Param.Value        $7=Asteroids
%Param.Value        $7=Planets
%Param.Value        $7=Comets
%Param.Value        $8=120 arcsec
%Param.Value        $8=60 arcsec
%Param.Value        $8=10 arcsec
%Param.Value        $8=1 arcsec
%Param.Value        $8=0 (no limit)
%ResultDataType     Mime(text/xml)
%VerboseDescr       Allows access to the SkyBoT database for search and identification of solar system objects
%Institute          Institut de mecanique celeste - Observatoire de Paris
%Doc.User           http://vo.imcce.fr/webservices/skybot
%Aladin.Label       SkyBoT
%Aladin.LabelPlane  SkyBoT $1
%Aladin.Filter      #Arrow of motion\nfilter Ast.Motion { draw ${Name};draw cross\n draw pm(5*${dRAcosDec}/cos(3.1416*${_DECJ2000}/180),5*${dDEC}) }
%Aladin.Filter      #Object name\nfilter Ast.Name { draw ${Name} }
%Aladin.Filter      #Object class\nfilter Ast.Class { ${Class}="NEA>Atira" {draw green square}\n${Class}="NEA>Aten" {draw yellow square}\n${Class}="NEA>Apollo" {draw blue square}\n${Class}="NEA>Amor" {draw orange square}\n${Class}="Mars-Crosser>Deep" {draw red square}\n${Class}="Mars-Crosser>Shallow" {draw red cross}\n${Class}="Hungaria" {draw cyan cross}\n${Class}="MB>IMB" {draw green cross}\n${Class}="MB>MMB" {draw blue cross}\n${Class}="MB>OMB" {draw red cross}\n${Class}="MB>Cybele" {draw orange cross}\n${Class}="MB>Hilda" {draw cyan square}\n${Class}="Trojan" {draw pink square}\n${Class}="Centaur" {draw gray oval}\n${Class}="KBO>Classical" {draw lightGray rhomb}\n${Class}="KBO>Plutino" {draw white rhomb}\n${Class}="KBO>SDO" {draw darkGray rhomb} }
%Aladin.Filter      #Magnitude circle\nfilter Ast.Mag { draw circle(-${Mv}) }
%Aladin.Filter      #Position error & arrow of motion\nfilter Ast.ErrorPosMotion { draw cross\n draw circle(${ErrPos})\n draw pm(5*${dRAcosDec}/cos(3.1416*${_DECJ2000}/180),5*${dDEC}) }
%Aladin.Filter      #Position error\nfilter Ast.ErrorPos { draw\n draw circle(${ErrPos}) }
%Aladin.Filter      #Geocentric distance\nfilter Ast.Dist.Geo { draw circle(${Dgeo}) }
%Aladin.Filter      #Heliocentric distance\nfilter Ast.Dist.Helio { draw circle(${Dhelio}) }

%ActionName         SkyBot.resolver
%Description        Solar system object resolver from IMCCE (name+epoch)
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1259754410  2009/12/02 13:46:50
%Url                http://vo.imcce.fr/webservices/skybot/skybotresolver_query.php?-ep=$2&-obj=$1&-mime=text&-out=basic
%Param.Description  $1=Object name
%Param.Description  $2=Epoch
%ResultDataType     Mime(text/xml)

%ActionName         SkyView
%Description        SkyView Virtual Observatory
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      0  1998/02/16 18:24:43
%Url                http://skyview.gsfc.nasa.gov/cgi-bin/nnskcall.pl?VCOORD=$1&SURVEY=$2&SCOORD=Equatorial&EQUINX=2000&MAPROJ=Gnomonic&SFACTR=Default&ISCALN=Log%2810%29&GRIDDD=No
%Param.Description  $2=Survey
%Param.DataType     $1=J2000
%Param.Value        $2=Digitized Sky Survey
%Param.Value        $2=IRAS 12 micron
%ResultDataType     Mime(text/html)
%Doc.User           http://skyview.gsfc.nasa.gov/help/help.html

%ActionName         Skyview
%Description        HEASARC SkyView image server
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1536914271  2018/09/14 10:37:51
%Url                https://skyview.gsfc.nasa.gov/cgi-bin/images?Sampler=$8&Coordinates=$6&Projection=$5&SURVEY=$4&Position=$1&Size=$3&Pixels=$2&Rotation=$7&RETURN=FITS
%Param.Description  $1=Target or coordinates
%Param.Description  $2=Pixels (n or n,m)
%Param.Description  $4=Surveys
%Param.Description  $3=Size deg. (n or n,m)
%Param.Description  $5=Projection
%Param.Description  $6=Coordinates
%Param.Description  $7=Rotation
%Param.Description  $8=Sampling
%Param.DataType     $1=Target(COO|SIMBAD)
%Param.Value        $2=300
%Param.Value        $3=Default
%Param.Value        $4=Fermi 5
%Param.Value        $4=Fermi 4
%Param.Value        $4=Fermi 3
%Param.Value        $4=Fermi 2
%Param.Value        $4=Fermi 1
%Param.Value        $4=EGRET (3D)
%Param.Value        $4=EGRET >100 MeV
%Param.Value        $4=EGRET <100 MeV
%Param.Value        $4=COMPTEL
%Param.Value        $4=INT GAL 17-35 Flux
%Param.Value        $4=INT GAL 17-60 Flux
%Param.Value        $4=INT GAL 35-80 Flux
%Param.Value        $4=INTEGRAL/SPI GC
%Param.Value        $4=GRANAT/SIGMA
%Param.Value        $4=RXTE Allsky 3-20keV
%Param.Value        $4=RXTE Allsky 3-8keV
%Param.Value        $4=RXTE Allsky 8-20keV
%Param.Value        $4=BAT SNR 14-195
%Param.Value        $4=BAT SNR 14-20
%Param.Value        $4=BAT SNR 20-24
%Param.Value        $4=BAT SNR 24-35
%Param.Value        $4=BAT SNR 35-50
%Param.Value        $4=BAT SNR 50-75
%Param.Value        $4=BAT SNR 75-100
%Param.Value        $4=BAT SNR 100-150
%Param.Value        $4=BAT SNR 150-195
%Param.Value        $4=RASS-Cnt Soft
%Param.Value        $4=RASS-Cnt Hard
%Param.Value        $4=RASS-Cnt Broad
%Param.Value        $4=PSPC 2.0 Deg-Int
%Param.Value        $4=PSPC 1.0 Deg-Int
%Param.Value        $4=PSPC 0.6 Deg-Int
%Param.Value        $4=HRI
%Param.Value        $4=HEAO 1 A-2
%Param.Value        $4=RASS Background 1
%Param.Value        $4=RASS Background 2
%Param.Value        $4=RASS Background 3
%Param.Value        $4=RASS Background 4
%Param.Value        $4=RASS Background 5
%Param.Value        $4=RASS Background 6
%Param.Value        $4=RASS Background 7
%Param.Value        $4=GALEX Near UV
%Param.Value        $4=GALEX Far UV
%Param.Value        $4=ROSAT WFC F1
%Param.Value        $4=ROSAT WFC F2
%Param.Value        $4=EUVE 83 A
%Param.Value        $4=EUVE 171 A
%Param.Value        $4=EUVE 405 A
%Param.Value        $4=EUVE 555 A
%Param.Value        $4=DSS
%Param.Value        $4=DSS1 Blue
%Param.Value        $4=DSS1 Red
%Param.Value        $4=DSS2 Red
%Param.Value        $4=DSS2 Blue
%Param.Value        $4=DSS2 IR
%Param.Value        $4=SDSSg
%Param.Value        $4=SDSSi
%Param.Value        $4=SDSSr
%Param.Value        $4=SDSSu
%Param.Value        $4=SDSSz
%Param.Value        $4=SDSSdr7g
%Param.Value        $4=SDSSdr7i
%Param.Value        $4=SDSSdr7r
%Param.Value        $4=SDSSdr7u
%Param.Value        $4=SDSSdr7z
%Param.Value        $4=Mellinger Red
%Param.Value        $4=Mellinger Green
%Param.Value        $4=Mellinger Blue
%Param.Value        $4=NEAT
%Param.Value        $4=H-Alpha Comp
%Param.Value        $4=SHASSA H
%Param.Value        $4=SHASSA CC
%Param.Value        $4=SHASSA C
%Param.Value        $4=SHASSA Sm
%Param.Value        $4=2MASS-J
%Param.Value        $4=2MASS-H
%Param.Value        $4=2MASS-K
%Param.Value        $4=UKIDSS-J
%Param.Value        $4=UKIDSS-H
%Param.Value        $4=UKIDSS-K
%Param.Value        $4=WISE 3.4
%Param.Value        $4=WISE 4.6
%Param.Value        $4=WISE 12
%Param.Value        $4=WISE 22
%Param.Value        $4=IRIS 12
%Param.Value        $4=IRIS 25
%Param.Value        $4=IRIS 60
%Param.Value        $4=IRIS 100
%Param.Value        $4=SFD 100m
%Param.Value        $4=SFD Dust Map
%Param.Value        $4=IRAS 12 micron
%Param.Value        $4=IRAS 25 micron
%Param.Value        $4=IRAS 60 micron
%Param.Value        $4=IRAS 100 micron
%Param.Value        $4=Planck 857
%Param.Value        $4=Planck 545
%Param.Value        $4=Planck 353
%Param.Value        $4=Planck 217
%Param.Value        $4=Planck 143
%Param.Value        $4=Planck 100
%Param.Value        $4=Planck 070
%Param.Value        $4=Planck 044
%Param.Value        $4=Planck 030
%Param.Value        $4=WMAP ILC
%Param.Value        $4=WMAP Ka
%Param.Value        $4=WMAP K
%Param.Value        $4=WMAP Q
%Param.Value        $4=WMAP V
%Param.Value        $4=WMAP W
%Param.Value        $4=COBE DIRBE/AAM
%Param.Value        $4=COBE DIRBE/ZSMA
%Param.Value        $4=GB6 (4850Mhz)
%Param.Value        $4=VLA FIRST (1.4 Ghz)
%Param.Value        $4=NVSS
%Param.Value        $4=Stripe82VLA
%Param.Value        $4=1420Mhz (Bonn)
%Param.Value        $4=nH
%Param.Value        $4=SUMSS 843 MHz
%Param.Value        $4=0408Mhz
%Param.Value        $4=WENSS
%Param.Value        $4=CO
%Param.Value        $4=VLSSr
%Param.Value        $4=0035MHz
%Param.Value        $4=GOODS: Chandra ACIS HB
%Param.Value        $4=GOODS: Chandra ACIS FB
%Param.Value        $4=GOODS: Chandra ACIS SB
%Param.Value        $4=GOODS: VLT VIMOS U
%Param.Value        $4=GOODS: VLT VIMOS R
%Param.Value        $4=GOODS: HST ACS B
%Param.Value        $4=GOODS: HST ACS V
%Param.Value        $4=GOODS: HST ACS I
%Param.Value        $4=GOODS: HST ACS Z
%Param.Value        $4=Hawaii HDF U
%Param.Value        $4=Hawaii HDF B
%Param.Value        $4=Hawaii HDF V0201
%Param.Value        $4=Hawaii HDF V0401
%Param.Value        $4=Hawaii HDF R
%Param.Value        $4=Hawaii HDF I
%Param.Value        $4=Hawaii HDF z
%Param.Value        $4=Hawaii HDF HK
%Param.Value        $4=GOODS: HST NICMOS
%Param.Value        $4=GOODS: VLT ISAAC J
%Param.Value        $4=GOODS: VLT ISAAC H
%Param.Value        $4=GOODS: VLT ISAAC Ks
%Param.Value        $4=HUDF: VLT ISAAC Ks
%Param.Value        $4=GOODS: Spitzer IRAC 3.6
%Param.Value        $4=GOODS: Spitzer IRAC 4.5
%Param.Value        $4=GOODS: Spitzer IRAC 5.8
%Param.Value        $4=GOODS: Spitzer IRAC 8.0
%Param.Value        $4=GOODS: Spitzer MIPS 24
%Param.Value        $4=GOODS: Herschel 100
%Param.Value        $4=GOODS: Herschel 160
%Param.Value        $4=GOODS: Herschel 250
%Param.Value        $4=GOODS: Herschel 350
%Param.Value        $4=GOODS: Herschel 500
%Param.Value        $4=CDFS: LESS
%Param.Value        $4=GOODS: VLA North
%Param.Value        $5=Tan
%Param.Value        $5=Sin
%Param.Value        $5=Ait
%Param.Value        $5=Car
%Param.Value        $6=J2000
%Param.Value        $6=B1950
%Param.Value        $6=Galactic
%Param.Value        $6=ICRS
%Param.Value        $7=0
%Param.Value        $8=NN
%Param.Value        $8=LI
%Param.Value        $8=Lanczos
%Param.Value        $8=Clip
%ResultDataType     Mime(image/fits)
%Doc.User           http://skyview.gsfc.nasa.gov/
%Aladin.Label       SkyView+
%Aladin.Logo        SkyViewLogo.gif
%Aladin.LabelPlane  Skw+ $4
%Aladin.MenuNumber  I5

%ActionName         StarBits
%Description        StarBits home page
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/starbits.html
%ResultDataType     Mime(text/html)

%ActionName         StarBits.query
%Description        StarBits query by abbreviation (in Star*s Family)
%Owner              CDS'misc
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/sf-bin/starbits?$1
%Param.Description  $1=Abbreviation
%Param.DataType     $1=query/keywords
%Test               param="CDS" pattern="Centre de Don"
%ResultDataType     Mime(text/html)

%ActionName         StarHeads
%Description        StarHeads home page
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/starheads.html
%ResultDataType     Mime(text/html)

%ActionName         StarHeads.query
%Description        StarHeads query by last name
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/sf-bin/starheads?$1
%Param.Description  $1=Author name
%Param.DataType     $1=query/name
%Test               param="egret" pattern="Daniel"
%ResultDataType     Mime(text/html)

%ActionName         StarPages StarsFamily
%Description        Home page of the Star*s Family
%Owner              CDS'misc
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/starpages.html
%DefaultAnchorText  <B>S</B>tarPages
%FullTextResult     <A HREF="$url" target="_top">$text</A>
%Test               noparam
%ResultDataType     Mime(text/html)

%ActionName         StarWorlds
%Description        StarWorlds home page
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/starworlds.html
%ResultDataType     Mime(text/html)

%ActionName         StarWorlds.query
%Description        StarWorlds query  (in Star*s Family)
%Owner              CDS'misc
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/sf-bin/starworlds?word=Embedded+string&case=Case+insensitive&isindex=$1
%Param.Description  $1=a world
%Param.DataType     $1=query/keywords
%Test               param="CDS" pattern="Centre de Don"
%ResultDataType     Mime(text/html)

%ActionName         TAPVizieR.home
%Description        TAPVizieR web page
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1640253424  2021/12/23 11:57:04
%Url                http://tapvizier.cds.unistra.fr
%FullTextResult     <a href='$url/adql/' alt='TAP VizieR'>TAP VizieR</a>

%ActionName         TIPbase.service
%Description        TIPbase/TOPbase
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://cds.unistra.fr/cgi-bin/tipbase/tipbase.sh?$1&$2&$3&$4&$5&$6&$7&$8&$9&$10
%Test               param="viw=0 mod=0 nz1=1 nz2=1 ne1=1 ne2=28 li1=0 li2=0 lj1=0 lj2=0" pattern="href"

%ActionName         TOPCAT
%Description        Graphical viewer and editor for tabular data
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1634041411  2021/10/12 14:23:31
%VerboseDescr       TOPCAT is an interactive graphical viewer and editor for tabular data. Its aim is to provide most of the facilities that astronomers need for analysis and manipulation of source catalogues and other tables, though it can be used for non-astronomical data as well. It understands a number of different astronomically important formats (including FITS, VOTable and CDF) and more formats can be added. It is especially good at interactive exploration of large (multi-million row, lots of columns) tables.\nIt offers a variety of ways to view and analyse tables, including a browser for the cell data themselves, viewers for information about table and column metadata, and facilities for sophisticated interactive 1-, 2-, 3- and higher-dimensional visualisation, calculating statistics and joining tables using flexible matching algorithms. Using a powerful and extensible Java-based expression language new columns can be defined and row subsets selected for separate analysis. Table data and metadata can be edited and the resulting modified table can be written out in a wide range of output formats.
%Institute          Starlink & AstroGrid project (UK)
%Copyright          TOPCAT is available under the terms of the GNU General Public License
%Doc.User           http://www.star.bris.ac.uk/~mbt/topcat/
%ReleaseNumber      4.8-1 (lite)
%Jar                http://www.star.bris.ac.uk/~mbt/topcat/topcat-lite.jar
%JavaParam          -mx256m -jar topcat-lite.jar
%Aladin.Activated   Yes
%Aladin.VOLabel     TOPCAT interactive graphical viewer and editor for tabular data

%ActionName         Terapix.home
%Description        Terapix (IAP)
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1  2001/11/21 10:52:58
%Url                http://terapix.iap.fr/
%DefaultAnchorText  Terapix

%ActionName         Thermo
%Description        Temperature salle machine
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1311685586  2011/07/26 15:06:26
%Url                http://alasky.u-strasbg.fr/cgi/thermo
%Test               noparam pattern="Ca roule"
%ResultType         Mime(text/plain)

%ActionName         Tut.logo.mini Tut.logo
%Description        Dictionary logo
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1277298706  2010/06/23 15:11:46
%FullTextResult     <IMG SRC="<&CDSheadU>tut_40x35.png" ALT="Tutorial">
%ResultDataType     Mime(image/png)

%ActionName         TwikiCDS
%Description        Twiki du CDS
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1536073942  2018/09/04 17:12:22
%Url                http://cloud-wiki.u-strasbg.fr/status/TWikiCDS
%Test               param="noparam pattern=\"RUN\""
%ResultDataType     Mime(text/html)

%ActionName         UCD.WS
%Description        UCD resolver by Web services
%Owner              CDS'ws
%DistribDomain      CDS
%VersionNumber      1373967572  2013/07/16 11:39:32
%Url                http://cdsws.u-strasbg.fr/axis/services/UCD?$1
%Test               param="wsdl" pattern="UCDofCatalogResponse"
%ResultDataType     soap
%Doc.Technical      

%ActionName         UCD.doc.w
%Description        UCD documentation
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1630681033  2021/09/03 16:57:13
%FullTextResult     https://cds.unistra.fr/doc/UCD/

%ActionName         UCD.explain
%Description        Explain one UCD (definitions and statistics)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/UCD/cgi-bin/ucd_stats?leaf=$1
%Param.Description  $1=A UCD, e.g.  EXTENSION_FWHM_MAJ
%ResultDataType     Mime(text/html)

%ActionName         UDS.home UdS.home
%Description        Universite de Strasbourg home page
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1340094371  2012/06/19 10:26:11
%Url                http://www.unistra.fr/
%DefaultAnchorText  UdS

%ActionName         UGuide
%Description        Access to SIMBAD user's guide
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188913090  2007/09/04 15:38:10
%Url                <&SimbadGuide>/index.htx
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         UGuideEntry
%Description        Access to an individual page of the user's guide
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188913090  2007/09/04 15:38:10
%Url                <&SimbadGuide>/$1
%Param.Description  $1=User's guide chapter
%Test               param="06"
%ResultDataType     Mime(text/html)

%ActionName         UKIDSS
%Description        The UKIRT DR9 Infrared Deep Sky Survey
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1507560157  2017/10/09 16:42:37
%Url                http://wfaudata.roe.ac.uk/ukidssdr9-siap/?POS=$1,$2&SIZE=$3&FORMAT=image/fits
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%Param.Value        $3=0.17
%ResultDataType     Mime(sia/xml)
%VerboseDescr       UKIDSS is the next generation near-infrared sky survey, the successor to 2MASS. UKIDSS began in May 2005 and will survey 7500 square degrees of the Northern sky, extending over both high and low Galactic latitudes, in JHK to K=18.3. This depth is three magnitudes deeper than 2MASS. UKIDSS will be the true near-infrared counterpart to the Sloan survey, and will produce as well a panoramic clear atlas of the Galactic plane. In fact UKIDSS is made up of five surveys and includes two deep extra-Galactic elements, one covering 35 square degrees to K=21, and the other reaching K=23 over 0.77 square degrees.
%Institute          WFAU, Institute for Astronomy, University of Edinburgh
%Aladin.Profile     >6.9
%Aladin.Profile     <10
%Aladin.MenuNumber  I10
%Aladin.Label       UKIDSS
%Aladin.LabelPlane  UKIDSS $1 $2
%Aladin.Logo        UKIDSSLogo.gif
%Doc.user           http://www.ukidss.org/

%ActionName         ULP.logo
%Description        Logo of Universite Louis Pasteur de Strasbourg
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/Icons/Ulp.small.gif
%FullTextResult     <IMG SRC="$1" ALIGN="middle" ALT="ULP logo">
%ResultDataType     Mime(image/gif)

%ActionName         URLquery
%Description        Help page for queries by URLs
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188913090  2007/09/04 15:38:10
%Url                <&SimbadHelp>=sim-url
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         UaiIdent
%Description        UAI identifier description.
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/uaident.htx
%ResultDataType     Mime(text/html)

%ActionName         Unit
%Description        Explanation and Combination of Physical Units
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                <&VizU>/viz-bin/Unit?$1
%Param.Description  $1=Complex unit, e.g. km/s/Mpc or more complex....
%Param.DataType     $1=U
%Test               param="km/s/Mpc" pattern="3.240.*Hz"
%ResultDataType     Mime(text/html)
%Doc.User           https://vizier.cds.unistra.fr/viz-bin/Unit

%ActionName         Units.list
%Description        List of the basic units in vizier and associated services
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://cdsarc.cds.unistra.fr/vizier/Units.htx
%ResultDataType     Mime(text/html)
%Doc.User           https://vizier.cds.unistra.fr/viz-bin/Unit

%ActionName         VI-137-FX.hpx
%Description        GAIA GUMS STARS progressive catalog
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1490859993  2017/03/30 09:46:33
%Url                http://cdsxmatch.u-strasbg.fr/HiPSCatService/GAIA_GUMS_STARS/
%Copyright          beta acces only
%Id                 VI/137/FX
%Aladin.Profile     >6.1 <8.159 beta
%Aladin.XLabel      GAIA GUMS FX
%Aladin.Tree        Progressive catalog
%Aladin.HpxParam    11 cat equatorial
%VerboseDesc        GAIA_GUMS_STARS hierarchical access

%ActionName         VLSSr
%Description        VLSSr Postage Stamp Server (VLA/NRAO)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576819358  2019/12/20 07:22:38
%Url                http://www.cv.nrao.edu/cgi-bin/newVLSSpostage.pl?Equinox=J2000&PolType=$5&RA=$1&Dec=$2&Size=$3+$3&Cells=$4+$4&MAPROJ=$6&rotate=0.0&Type=$7
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Image Size (deg)
%Param.Description  $4=Pixel size (arcsec)
%Param.Description  $5=Polarization
%Param.Description  $6=Projection
%Param.Description  $7=Format
%Param.DataType     $1=Target(RAb)
%Param.DataType     $2=Target(DEb)
%Param.Value        $3=0.25
%Param.Value        $4=15.0
%Param.Value        $5=I - Stokes I
%Param.Value        $5=IQU
%Param.Value        $6=SIN - Sine
%Param.Value        $6=TAN - Tangent
%Param.Value        $6=ARC - Arc
%Param.Value        $6=NCP - North Celestial Pole
%Param.Value        $6=GLS - Global sinusoidial
%Param.Value        $6=MER - Mercator
%Param.Value        $6=AIT - Aitoff
%Param.Value        $6=STG - Stereographic
%Param.Value        $7=image/x-fits
%Param.Value        $7=image/jpeg
%ResultDataType     Mime(image/fits)
%Doc.User           http://www.cv.nrao.edu/vlss/VLSSpostage.shtml
%Aladin.Label       VLSSr Postage Stamp Server (VLA/NRAO)
%Aladin.LabelPlane  VLSSr
%Aladin.Menu        VLA...
%Aladin.Profile     <10.144

%ActionName         Vignettes.CDS
%Description        Vignette de densite des tables VizieR et de Simbad
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1507562904  2017/10/09 17:28:24
%SeeAction          Vignettes.CDS_0 availability=9999
%SeeAction          Vignettes.CDS_1 availability=9999

%ActionName         Viz.GCVS
%Description        Details for a Variable Star
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=GCVS/gcvs&GCVS=$1%20%2a$2
%Param.Description  $1=First part of name of variable star
%Param.Description  $2=Constellation name
%Param.DataType     $1=text
%Param.DataType     $2=text
%Test               param="R AND"
%Test               param="V1234 Cyg"
%ResultDataType     Mime(text/html)

%ActionName         Viz.GLU astroviz
%Description        Generation of the astroviz dic for Astrobrowse Usage
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO
%DistribDomain      SSDS.astronomy
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/viz-bin/vizglu?-pos&-all&-ApplicationField=Astrobrowse&$1
%DefaultAnchorText  Astroviz generation for Astrobrowse usage
%Param.Description  $1=-long if a long format is wished.
%ResultDataType     Mime(text/plain)

%ActionName         Viz.MP
%Description        VizieR Query for a Minor Planet
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=B/astorb/astorb&Planet=$1
%Param.DataType     $1=MP
%Test               param="4692"
%Test               param="1"
%Test               param="8443"
%ResultDataType     Mime(text/html)

%ActionName         Viz.asteroid
%Description        VizieR Query for an Asteroid, including trans-Uranian
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=B/astorb/astorb&Name==$1
%Param.DataType     $1=misc'query/keywords
%Test               param="\"2000 EB173\""
%ResultDataType     Mime(text/html)

%ActionName         Viz.comet
%Description        VizieR Query for a Comet (from its code)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=B/comets&Code==$1
%Param.DataType     $1=misc'query/keywords
%Test               param="19P"
%ResultDataType     Mime(text/html)

%ActionName         Viz.ftp
%Description        FTP service
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                ftp://cdsarc.cds.unistra.fr/
%Test               noparam pattern="incoming"
%ResultType         Mime(text/html);

%ActionName         Viz.logo
%Description        VizieR logo
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1708502034  2024/02/21 09:53:54
%Url                /vizier/vizier.png
%FullTextResult     <IMG SRC="$url" alt="vizier">
%ResultDataType     Mime(image/png)

%ActionName         Viz.logo.mini
%Description        VizieR logo
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1277298706  2010/06/23 15:11:46
%FullTextResult     <IMG SRC="<&CDSheadU>vizier_40x35.png" ALT="VizieR">
%ResultDataType     Mime(image/png)

%ActionName         Viz.logo.tiny
%Description        VizieR logo
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&CDSheadU>/vizier_20x18.png
%FullTextResult     <IMG SRC="$url" alt='vizier'>
%ResultDataType     Mime(image/png)

%ActionName         Viz.logos.cadc
%Description        ESO catalogues
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/
%FullTextResult     <a href='http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/' title='Data provided by CADC'><img class='logo-image' src='/vizier/logos/cadc.png' alt='CADC origin'/></a>

%ActionName         Viz.logos.eso
%Description        ESO catalogues
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.eso.org
%FullTextResult     <a href='http://www.eso.org' title='Data provided by ESO'><img class='logo-image' src='/vizier/logos/eso.png' alt='ESO origin'/></a>

%ActionName         Viz.monbigcat
%Description        VizieR big catalogs server in CDS (aserver+QueryCatDaemon)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1727798100  2024/10/01 17:55:00
%Url                http://vizcat.cds.unistra.fr/cgi-bin/qat2s.cgi?file=2mass&has_header=false&columns[cols][0]=%24%7B2MASS%7D&limit=1&print_header=false&recno=false&output[FullPrecSV]=%2C&cgi=false&mode=All
%Test               param=":" pattern="02595905"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.bigcat.md
%ResultType         Mime(text/html);

%ActionName         Viz.mondb
%Description        VizieR database monitor in CDS
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1664191194  2022/09/26 13:19:54
%Url                http://vizdata.cds.unistra.fr/pcds.log
%Test               param=":" pattern="SERVICE IS OK"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.service.md
%Doc.User           http://cdsarc.cds.unistra.fr/spv/
%ResultType         Mime(text/html);

%ActionName         Viz.mondb.local
%Description        VizieR local database monitor (cdsarc used by documentalists)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1663312410  2022/09/16 09:13:30
%Url                http://cdsarc.cds.unistra.fr/vizdb.log
%Test               param=":" pattern="SERVICE IS OK"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.service.md
%Doc.User           http://cdsarc.cds.unistra.fr/spv/
%ResultType         Mime(text/html);

%ActionName         Viz.mondbpool
%Description        VizieR database monitor in CDS (using pool)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1664191194  2022/09/26 13:19:54
%Url                http://vizdata.cds.unistra.fr/pcdspool.log
%Test               param=":" pattern="SERVICE IS OK"
%Doc.User           http://cdsarc.cds.unistra.fr/spv/
%ResultType         Mime(text/html);

%ActionName         Viz.monsesame
%Description        Sesame monitor
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://cdsarc.cds.unistra.fr/spv/monitorsesame.log
%Test               param=":" pattern="SERVICE IS OK"
%Doc.User           https://cdsarc.cds.unistra.fr/spv/
%ResultType         Mime(text/html);

%ActionName         Viz.monsubmit
%Description        VizieR table submission
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://cdsarc.cds.unistra.fr/vizier.submit/uws/admin?format=json
%Test               param=":" pattern="COMPLETED"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.cats.md
%ResultType         Mime(application/json);

%ActionName         Viz.montap
%Description        TAPVizieR monitor
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1713281778  2024/04/16 17:36:18
%Url                http://tapvizier.cds.unistra.fr/TAPVizieR/tap/availability
%Test               param=":" pattern=" available"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.tap.md
%ResultType         Mime(application/xml);

%ActionName         Viz.montapvizier1
%Description        TAPVizieR monitor node tapvizier1
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://tapvizier1.cds.unistra.fr/TAPVizieR/tap/availability
%Test               param=":" pattern=" available"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.tap.md
%ResultType         Mime(application/xml);

%ActionName         Viz.montapvizier2
%Description        TAPVizieR monitor node tapvizier2
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://tapvizier2.cds.unistra.fr/TAPVizieR/tap/availability
%Test               param=":" pattern=" available"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.tap.md
%ResultType         Mime(application/xml);

%ActionName         Viz.monvsearch
%Description        vsearch monitor (textual search)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://cdsarc.unistra.fr/viz-bin/cat?type=query&m=0..1&format=json&displayed_fields=id&query=redshift
%Test               param="::" pattern="_source"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.cats.md
%ResultType         Mime(application/json)

%ActionName         Viz.more
%Description        VizieR more links
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1592484190  2020/06/18 14:43:10
%FullTextResult      <div><div class='morelinks left' style='font-size:smaller'>\n<div class='title'>Tools related to VizieR</div>\n<ul>\n<li><div class='title'><a href='<&getcat,u>'>Catalogue collection</a> : </div>\n<div class='explain'>Search VizieR catalogues available via various services (FTP, VizieR, TAP, ...)</div>\n</li>\n<li><div class='title'><&Portal.home> : </div>\n<div class='explain'>Access CDS data including VizieR, Simbad and Aladin using the CDS portal</div>\n</li>\n<li><div class='title'><&VizieR.AssocData.home> : </div>\n<div class='explain'>Search Spectra, images in VizieR</div>\n</li>\n<li><div class='title'> <&VizieR.sed.home> : </div>\n<div class='explain'>Plot photometry (sed) including all VizieR</div>\n</li>\n<li><div class='title'><&TAPVizieR.home> : </div>\n<div class='explain'>query VizieR using ADQL (a SQL extension dedicated for astronomy)\n</div>\n</li>\n<li><div class='title'><&XMatch.home> : </div>\n<div class='explain'>fast cross-identification between any 2 tables, including VizieR catalogues, SIMBAD\n</div>\n</li>\n</ul>\n</div><div class='clear'> </div></div>

%ActionName         Viz.piwik
%Description        Piwik statistics
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1289398149  2010/11/10 16:09:09
%SeeAction          Viz.piwik.cds availability=7
%SeeAction          Viz.piwik.cfa availability=5
%SeeAction          Viz.piwik.adac availability=5
%SeeAction          Viz.piwik.cadc availability=1050
%SeeAction          Viz.piwik.uk availability=9999
%SeeAction          Viz.piwik.iucaa availability=7
%SeeAction          Viz.piwik.ru availability=9999
%SeeAction          Viz.piwik.ch availability=1050
%SeeAction          Viz.piwik.hw availability=9999

%ActionName         Viz4Sim
%Description        VizieR Output for Simbad
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      SSDS.astronomy
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/cgi-bin/VizieR?-4i&-out.form=a&-out.max=9999&-source=$1&$2&$3&$4&$5&$6&$7
%Param.Description  $1=Name of Catalog or Table
%Param.Description  $2=Any further VizieR Qualification
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="1239/hip_main"
%Test               param="HIP=57260"
%ResultDataType     Mime(text/html)

%ActionName         VizA.adac
%Description        VizieR Access (ADAC, Tokyo)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.nao.ac.jp/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.cadc
%Description        VizieR Access (CADC, Canada)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.hia.nrc.ca/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.cds Viz.home
%Description        VizieR service Access
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%DistribDomain      SSDS.astronomy
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://vizier.cds.unistra.fr/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)
%Doc.User           https://vizier.cds.unistra.fr/

%ActionName         VizA.cfa
%Description        VizieR Access (CFA, Harvard)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cfa.harvard.edu/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.ch
%Description        VizieR Access (Bejing Observatory, China)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.china-vo.org/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.hw
%Description        VizieR Access (UK Infra-red Telescope, Hawaii)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.ukirt.hawaii.edu/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.idia
%Description        VizieR Access (IDIA, South Africa)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1597408742  2020/08/14 14:39:02
%Url                http://vizier.idia.ac.za/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.iucaa
%Description        VizieR Access (IUCAA/Pune, India)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1578055097  2020/01/03 14:38:17
%Url                https://vizier.iucaa.in/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.ru
%Description        VizieR Access (INASAN, Moscow, Russia)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                https://vizier.inasan.ru/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.saao
%Description        VizieR Access (SAAO, South Africa)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1597408742  2020/08/14 14:39:02
%Url                http://vizier.idia.ac.za/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.uk
%Description        VizieR Access (Cambridge, UK)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.ast.cam.ac.uk/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizA.www VizA
%Description        VizieR service main Anchor (includes clones )
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR?$1
%DefaultAnchorText  <b>V</b>izieR
%FullTextResult     <a href="$url" target="_top">$text</a>
%Param.Description  $1=ASU parameters, e.g. -source=catalog&-c=target_position
%Test               param="-source=PMM" option="n"
%Test               param="-c.eq=now&-out.max=20" option="n"
%ResultDataType     Mime(text/html)

%ActionName         VizDensityMaps.HiPS
%Description        Retourne l'URL racine du HiPS de densité correspondant à la table VizieR demandé
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1677663158  2023/03/01 11:32:38
%Url                http://alasky.cds.unistra.fr/footprints/hips-density-maps/$1/$2
%Param.Description  $1= VizieR table identifier
%Param.Description  $2= path in HiPS structure
%Test               param="I/337/gaia properties" pattern="creator_did"

%ActionName         VizDetail.cds Viz.Detail
%Description        VizieR Query Detailed Page Result
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/viz-bin/VizieR-5?-source=$1&-out.add=.&$2&$3&$4
%Param.Description  $1=Name or Number of a Table
%Param.Description  $2=Full parameter for a query, e.g. HD=12345
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="GCVS \"GCVS=R *AND\""
%Test               param="I/239/hip_main HIP=9404"
%ResultDataType     Mime(text/html)

%ActionName         VizF
%Description        For conversion of <&VizF> into the root FTP address (bazaar clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1579782085  2020/01/23 14:21:25
%SeeAction          VizF.cds availability=7
%SeeAction          VizF.adac availability=5

%ActionName         VizF.http
%Description        For conversion of <&VizF> into the root FTP address (bazaar clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1584353002  2020/03/16 12:03:22
%SeeAction          VizF.cds.http availability=6
%SeeAction          VizF.adac availability=5

%ActionName         VizFind.www VizFind VizirFind VizierFind FindVizieR
%Description        VizieR Query of any catalogue by object name or coordinates (includes Clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR?-source=$1&-c=$2&-c.rm=$3&-out.add=_r&-sort=_r
%Param.Description  $1=Name or Number of a catalogue
%Param.Description  $2=Identification or J2000-position
%Param.Description  $3=Max distance from target position, in arcminutes
%Param.DataType     $1=E
%Param.DataType     $2=simbad'I
%Param.DataType     $2=J2000
%Test               param="HR M31"
%Test               param="III/135 01:23:45+12:25"
%Test               param="3135 01:23:45+12:25"
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.adac
%Description        VizieR service Home Page (ADAC, Tokyo)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.nao.ac.jp/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.cadc
%Description        VizieR service Home Page (CADC, Canada)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.hia.nrc.ca/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.cds VizHomePage
%Description        VizieR service Home Page (CDS, Strasbourg)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%DistribDomain      SSDS.astronomy
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.cfa
%Description        VizieR service Home Page (CFA, Harvard)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cfa.harvard.edu/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.ch
%Description        VizieR service Home Page (Bejing Astronomical Observatory, China)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.china-vo.org/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.hw
%Description        VizieR service Home Page (UK Infra-red Telescope, Hawaii)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.ukirt.hawaii.edu/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.idia
%Description        VizieR service Home Page (IDIA, South Africa)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1597408742  2020/08/14 14:39:02
%Url                http://vizier.idia.ac.za/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.iucaa
%Description        VizieR service Home Page (IUCAA/Pune, India)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1578055097  2020/01/03 14:38:17
%Url                https://vizier.iucaa.in/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.local
%Description        VizieR Home Page (local service)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                /viz-bin/VizieR
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.ru
%Description        VizieR service Home Page (INASAN, Moscow, Russia)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                https://vizier.inasan.ru/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.saao
%Description        VizieR service Home Page (SAAO, South Africa)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1597408742  2020/08/14 14:39:02
%Url                http://vizier.idia.ac.za/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.uk
%Description        VizieR service Home Page (UK, Cambridge)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.ast.cam.ac.uk/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizHomePage.www
%Description        VizieR service Home Page (includes Clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/vizier/
%DefaultAnchorText  <b>V</b>izieR
%ResultDataType     Mime(text/html)

%ActionName         VizRecord.cds VizRecord Viz.Record
%Description        VizieR Query Detailed Page Result from a Recno
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=$1&-out.add=RAJ,DEJ,Glon,Glat&recno=$2
%Param.Description  $1=Name or Number of a Table
%Param.Description  $2=Record number within the table
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="2250 1234,1235"
%Test               param="I/239/hip_main 9398"
%ResultDataType     Mime(text/html)

%ActionName         VizU
%Description        For conversion of <&VizU> into the root URL. (General access)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1630393719  2021/08/31 09:08:39
%SeeAction          VizU.cds availability=6
%SeeAction          VizU.cfa availability=7
%SeeAction          VizU.adac availability=5
%SeeAction          VizU.cadc availability=1050
%SeeAction          VizU.iucaa availability=6
%SeeAction          VizU.ru availability=9999
%SeeAction          VizU.ch availability=1051
%SeeAction          VizU.saao availability=8

%ActionName         VizU.hw
%Description        For conversion of <&VizU> into the root URL
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://www.ukirt.hawaii.edu/viz-bin/VizieR
%DefaultAnchorText  Hawai VizieR mirror
%FullTextResult     http://www.ukirt.hawaii.edu
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.Technical       https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.service.md

%ActionName         VizU.idia
%Description        For conversion of <&VizU> into the root URL
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://vizier.idia.ac.za/viz-bin/VizieR
%DefaultAnchorText  IDIA VizieR mirror
%FullTextResult     http://vizier.idia.ac.za
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.Technical       https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.service.md

%ActionName         VizU.local
%Description        VizieR local service
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%DistribDomain      SSDS.astronomy
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://cdsarc.cds.unistra.fr/viz-bin/VizieR
%DefaultAnchorText  CDS
%FullTextResult     https://cdsarc.cds.unistra.fr
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.User           https://cdsarc.cds.unistra.fr/cgi-bin/Help?VizieR/intro

%ActionName         VizU.uk
%Description        For conversion of <&VizU> into the root URL
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                http://vizier.ast.cam.ac.uk/viz-bin/VizieR
%DefaultAnchorText  Cambridge UK
%FullTextResult     http://vizier.ast.cam.ac.uk
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.Technical       https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.service.md

%ActionName         VizX
%Description        For conversion of <&VizX> into the root URL. (XML access)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO ExceptField= DefaultAnchorText
%VersionNumber      1630393719  2021/08/31 09:08:39
%SeeAction          VizX.cds availability=6
%SeeAction          VizU.cfa availability=7
%SeeAction          VizU.adac availability=5
%SeeAction          VizU.cadc availability=1050
%SeeAction          VizU.iucaa availability=6
%SeeAction          VizU.ch availability=1051
%SeeAction          VizU.saao availability=8

%ActionName         VizieR Vizir
%Description        VizieR Query Form for a Catalogue (by acronym or number)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      SSDS.astronomy
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR?-source=$1&$2
%Param.Description  $1=Name or Number of a catalogue
%Param.DataType     $1=E
%Test               param="HR"
%Test               param="I/239/hip_main  -c=0+90"
%Test               param="III/135  HD=226868"
%Test               param="3135"
%ResultDataType     Mime(text/html)

%ActionName         VizieR-c
%Description        VizieR Query on all or Wavelength-defined Catalogues
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-4?-c=$1&-c.rs=$2&-kw.Wavelength=$3&-out.add=.&-sort=_r&-out.form=H&$4
%Param.Description  $1=Identification or J2000-position
%Param.Description  $2=Max distance from target position, in arcminutes (default10)
%Param.Description  $3=Wavelength Keyword, in Set: Radio / IR / optical / UV / EUV / X-ray / Gamma-ray
%Param.Description  $4=Additional option
%Param.DataType     $1=simbad'I
%Param.DataType     $1=J2000
%Param.DataType     $3=misc'query/keywords
%Test               param="HD226868 10 X-ray"
%Test               param="M101"
%Test               param="01:23:45+12:25 5 optical"
%ResultDataType     Mime(text/html)

%ActionName         VizieR.AssocData.ObsTAP
%Description        VizieR ObsTAP service
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1587733836  2020/04/24 15:10:36
%Url                https://cdsarc.cds.unistra.fr/saadavizier.tap/tap/$1
%Param.Description  $1=TAP service + arguments: e.g.: sync?request=doQuery&phase=RUN&lang=adql&format=json&query=....
%Test               param="availability" pattern=".*available.*true.*"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.assocdata.md
%ResultType         Mime(text/html);

%ActionName         VizieR.AssocData.SIA
%Description        VizieR SIA service
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1587733836  2020/04/24 15:10:36
%Url                https://cdsarc.cds.unistra.fr/saadavizier/siaservice?collection=[vizier]&$1
%Param.Description  $1=SIA arguments
%Test               param="pos=0+0&size=0.1" pattern="QUERY_STATUS.*OK"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.assocdata.md
%ResultType         Mime(text/html);

%ActionName         VizieR.AssocData.SSA
%Description        VizieR SSA service
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1587733836  2020/04/24 15:10:36
%Url                https://cdsarc.cds.unistra.fr/saadavizier/ssaservice?collection=[vizier]&$1
%Param.Description  $1=SIA arguments
%Test               param="pos=0+10&size=0.05" pattern="QUERY_STATUS.*OK"
%Doc.Technical      https://gitlab.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.assocdata.md
%ResultType         Mime(text/html);

%ActionName         VizieR.AssocData.home
%Description        VizieR associated data web page
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638285499  2021/11/30 17:18:19
%Url                https://cdsarc.cds.unistra.fr/assocdata/
%FullTextResult     <a href='$url' alt='VizieR associated data'>Spectra, images in VizieR</a>

%ActionName         VizieR.AssocData.service
%Description        VizieR assoc data service (saada)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638285499  2021/11/30 17:18:19
%Url                https://cdsarc.cds.unistra.fr/saadavizier/

%ActionName         VizieR.Meta
%Description        Query the VizieR service to retrieve meta information\nabout the query specifications (currently in VOTable1.1)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/asu-xml/V1.1?-meta.aladin=all

%ActionName         VizieR.Meta2
%Description        Query the VizieR service to retrieve meta information\nabout the query specifications, following VOTable1.2 specs
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/asu-xml?-meta.aladin=all

%ActionName         VizieR.MetaCat
%Description        Query the VizieR service to retrieve catalogue name and description\naround a position (currently in VOTable1.1)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/asu-xml/V1.1?-meta&$1

%ActionName         VizieR.MetaCat2
%Description        Query the VizieR service to retrieve catalogue name and description\naround a position, following VOTable1.2 specs
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/asu-xml?-meta&$1

%ActionName         VizieR.QueryCat
%Description        QueryCat server (large tables service)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1598369844  2020/08/25 17:37:24
%SeeAction          VizieR.QueryCat.cds availability=9999
%SeeAction          VizieR.QueryCat.cds.http availability=0
%SeeAction          VizieR.QueryCat.iucaa availability=11
%SeeAction          VizieR.QueryCat.iucaa.http availability=11
%SeeAction          VizieR.QueryCat.idia availability=10
%SeeAction          VizieR.QueryCat.idia.http availability=11

%ActionName         VizieR.Tutorial
%Description        VizieR tutorial
%Owner              CDS'glu
%DistribDomain      CDS
%VersionNumber      1350312530  2012/10/15 16:48:50
%FullTextResult     <&CDS.Tutorial,u>#vizierTutorial
%ResultDataType     Mime(text/html)

%ActionName         VizieR.WS
%Description        VizieR access by Web services
%Owner              CDS'ws
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cdsws.u-strasbg.fr/axis/services/VizieR?$1
%Test               param="wsdl" pattern="cataloguesMetaDataResponse1"
%ResultDataType     soap
%Doc.Technical      http://cds.unistra.fr/cdsws/vizierAccess.gml

%ActionName         VizieR.cats
%Description        VizieR search for catalogues from name, words, position, ...
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-2?-meta.ucd&-meta.all&-source=$1&-c=$2&-c.r=$3
%Param.Description  $1=Name or Number of a catalogue, words from title, author names, etc...
%Param.Description  $2=Identification or J2000-position
%Param.Description  $3=Max distance from target position, in arcminutes
%Param.DataType     $1=misc'query/keywords
%Param.DataType     $1=E
%Param.DataType     $2=simbad'I
%Param.DataType     $2=J2000
%Test               param="\"Hipparcos\""
%Test               param="\"ROSAT bright sources\""
%ResultDataType     Mime(text/html)

%ActionName         VizieR.icon
%Description        VizieR icon
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://cds.unistra.fr/Icons/vizier_tiny.gif
%FullTextResult     <IMG SRC="$1" ALIGN="middle" ALT="Vizier">
%ResultDataType     Mime(image/gif)

%ActionName         VizieR.licences
%Description        Rules of usage for VizieR data
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1630681033  2021/09/03 16:57:13
%Url                https://cds.unistra.fr/vizier-org/licences_vizier.html
%FullTextResult     <a href='https://cds.unistra.fr/vizier-org/licences_vizier.html'>Rules of usage for VizieR data</a>

%ActionName         VizieR.local
%Description        VizieR "Local" Query Form for a Catalogue (by acronym or number, with debugging details)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      SSDS.astronomy
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=$1&$2
%Param.Description  $1=Name or Number of a catalogue
%Param.DataType     $1=E
%Test               param="HR"
%Test               param="I/239/hip_main"
%Test               param="III/135"
%Test               param="3135"
%ResultDataType     Mime(text/html)

%ActionName         VizieR.logo
%Description        VizieR logo.
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1268472392  2010/03/13 11:26:32
%SeeAction          VizieR.logo.viz availability=9999
%SeeAction          VizieR.logo.rel availability=9999
%SeeAction          VizieR.logo.abs availability=7

%ActionName         VizieR.sed sed.xml
%Description        Query the VizieR service around a position and get fluxes
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1706686550  2024/01/31 09:35:50
%Url                <&VizU>/viz-bin/sed?-c=$1&-c.rs=$2
%Param.Description  $1=Identification or J2000-position
%Param.Description  $2=Max distance from target position, in arcsec (default=5")
%Param.DataType     $1=simbad'I
%Test               param="M2 2" pattern="<TD>"
%ResultDataType     Mime(text/xml)
%%U                 https://cdsarc.cds.unistra.fr/viz-bin/sed?-c=$1&-c.rs=$2

%ActionName         VizieR.sed.home
%Description        Photometry (SED) VizieR
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1648019697  2022/03/23 09:14:57
%Url                https://vizier.cds.unistra.fr/vizier/sed/?-c=$1&-c.rs=$2
%FullTextResult     <a href='https://vizier.cds.unistra.fr/vizier/sed/'>Photometry viewer</a>
%Param.Description  $1= target (object name or position)
%Param.Description  $2= radius in arcsec
%ResultDataType     Mime(text/html)

%ActionName         VizieR.sed.logo
%Description        VizieR SED logo
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&CDSheadU>/sed-icon.png
%FullTextResult     <img src='$url' alt='VizieR SED'/>
%ResultDataType     Mime(image/png)

%ActionName         VizieR.votable.meta
%Description        Query the VizieR service to retrieve catalogs in VOTable format
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/votable?-meta=a&-source=$1&-c=$2&-c.r=$3
%Param.Description  $1=Name or Number of a catalogue, or words defining catalog(s)
%Param.Description  $2=Identification or J2000-position
%Param.Description  $3=Max distance from target position, in arcminutes
%Param.DataType     $1=E
%Param.DataType     $2=simbad'I
%Param.DataType     $2=J2000
%Test               param="HR M31"
%Test               param="III/135 01:23:45+12:25"
%Test               param="3135 01:23:45+12:25"
%ResultDataType     Mime(text/xml)

%ActionName         VizieR.words.www VizieR.words
%Description        VizieR Query Form for catalogues selected by keywords (includes Clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-2?-meta.ucd&-meta.all&-words=$1
%Param.Description  $1=Words from title, author names, etc...
%Param.DataType     $1=misc'query/keywords
%Test               param="\"Hipparcos\""
%Test               param="\"ROSAT bright sources\""
%ResultDataType     Mime(text/html)

%ActionName         VizieRAssocData
%Description        VizieR Associated Data - Aladin Desktop access
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1641283844  2022/01/04 10:10:44
%Url                https://tapvizier.cds.unistra.fr/TAPVizieR/tap/sync?REQUEST=doQuery&LANG=ADQL&MAXREC=2000000&QUERY=SELECT+TOP+999+*+FROM+%22B%2Fassocdata%2Fobscore%22+WHERE+obs_collection='$4'+and+1=CONTAINS(POINT('ICRS',RAJ2000,DEJ2000),CIRCLE('ICRS',$1,$2,$3))
%Param.Description  $1=Right Ascension
%Param.Description  $2=Declination
%Param.Description  $3=Radius in deg
%Param.Description  $4=Catalog ID
%Param.DataType     $1=Target(RAd)
%Param.DataType     $2=Target(DEd)
%Param.DataType     $3=Field(RADIUSd)
%ResultDataType     Mime(text/xml)
%Aladin.Menu        IVOA...
%Aladin.XLabel      VizieR associated data
%Aladin.LabelPlane  $4
%Aladin.Profile     >11.052

%ActionName         VizieRXML++
%Description        Query the VizieR service to retrieve catalogs in XML VOTable(CSV) format
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1342171517  2012/07/13 11:25:17
%Url                <&VizU>/viz-bin/votable?-source=$1&-c=$2&-out.add=_RAJ,_DEJ&-oc.form=dm&-out.meta=DhuL&-out.max=999999&-c.rm=$3&-out=_VizieR,*Mime(image/fits),*&-mime=TSV&$4

%ActionName         VizieRXML.rm
%Description        Query the VizieR service to retrieve catalogs in XML format (by radius)
%Owner              CDS'aladin
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1342171517  2012/07/13 11:25:17
%Url                <&VizU>/viz-bin/asu-xml?-source=$1&-c=$2&-out.add=_RAJ,_DEJ&-oc.form=dm&-out.meta=DhuUL&-out.max=unlimited&-c.rm=$3&-out=*Mime(image/fits),*&$4

%ActionName         WDS.home
%Description        World Data System (WDS) home page.
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1622797670  2021/06/04 11:07:50
%Url                https://www.worlddatasystem.org/
%DefaultAnchorText  WDS

%ActionName         WEBDA.cl
%Description        Get info about one cluster from WEBDA
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.univie.ac.at/webda//cgi-bin/ocl_page.cgi?cluster=$1
%Param.Description  $1=I
%Param.Value        $1=NGC 6383
%ResultDataType     Mime(text/html)

%ActionName         WEBDA.home
%Description        Home page of the WEBDA (Base Donnees Amas)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.univie.ac.at/webda/
%ResultDataType     Mime(text/html)

%ActionName         WFPC2.alist
%Description        Get List of datasets making one WFPC2 Association
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://cadcwww.hia.nrc.ca/cadcbin/wdb/hst/science_members_wfpc2_r1/query?asn_id=$1
%Param.Description  $1=filename
%Param.Value        $1=U23G0103B
%ResultDataType     Mime(text/html)
%Copyright          Canadian Astronomical Data Centre (CADC)

%ActionName         WFPC2.fits
%Description        Get Images of WFPC2 from CADC
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/getData?archive=HSTCA&file_id=$1_science_drz_sci
%Param.Description  $1=filename
%Param.Value        $1=U23G0103B
%ResultDataType     Mime(image/fits)
%Copyright          Canadian Astronomical Data Centre (CADC)

%ActionName         WISE.IRSA
%Description        IRSA server (displays WISE images)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://irsa.ipac.caltech.edu/applications/wise/#id=Hydra_wise_wise_1&DoSearch=true&schema=allsky-4band&intersect=CENTER&subsize=$3&mcenter=mcen&band=1,2,3,4&dpLevel=3a&UserTargetWorldPt=$1;$2;EQ_J2000&SimpleTargetPanel.field.resolvedBy=simbadthenned&coaddId=&projectId=wise&searchName=wise_1&startIdx=0&pageSize=0&shortDesc=Position&isBookmarkAble=true&isDrillDownRoot=true&isSearchResult=true
%Param.Description  $1=Right Ascension (J2000), decimal degrees
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.Description  $3=Box size, degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=289.3833
%Param.Value        $2=11.9672
%Param.Value        $3=0.1667
%ResultDataType     Mime(text/html)

%ActionName         WISE.IRSA.ALLWISE
%Description        IRSA server (displays WISE images)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://irsa.ipac.caltech.edu/applications/wise/#id=Hydra_wise_wise_1&DoSearch=true&schema=allwise-multiband&intersect=CENTER&subsize=$3&mcenter=mcen&band=1,2,3,4&dpLevel=3a&UserTargetWorldPt=$1;$2;EQ_J2000&SimpleTargetPanel.field.resolvedBy=simbadthenned&coaddId=&projectId=wise&searchName=wise_1&startIdx=0&pageSize=0&shortDesc=Position&isBookmarkAble=true&isDrillDownRoot=true&isSearchResult=true
%Param.Description  $1=Right Ascension (J2000), decimal degrees
%Param.Description  $2=Declination (J2000), decimal degrees
%Param.Description  $3=Box size, degrees
%Param.DataType     $1=Coo(J2000,RAdeg)
%Param.DataType     $2=Coo(J2000,DEdeg)
%Param.Value        $1=289.3833
%Param.Value        $2=11.9672
%Param.Value        $3=0.1667
%ResultDataType     Mime(text/html)

%ActionName         WSRT
%Description        Westerbork Synthesis Radio Telescope (WSRT) observations archive
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      0  1998/02/16 18:24:43
%Url                http://www.nfra.nl/scibin/qed?select=observation&seqnumber=&project=&source=$1&ra=&dec=&equinox=B1950&system=Equatorial+FK5&obs_date=&duration=&frequency=&format=m&volume=
%Param.DataType     $1=CDS'simbad'I
%ResultDataType     Mime(text/html)
%Doc.User           http://www.nfra.nl/scissor/rdb/observation.frm
%Doc.User           http://www.nfra.nl/scissor/doc/scissor.html

%ActionName         WSimbad Simbad SIMBAD
%Description        Simbad home page
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1359471697  2013/01/29 17:01:37
%SeeAction          WSimbad.fr availability=7
%SeeAction          WSimbad.us availability=5

%ActionName         WSimbadFunctions
%Description        Description of SIMBAD on the web functionalities
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/WSimbad.htx
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         WSimbadHistory
%Description        Description of SIMBAD on the web history and new features
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/WSimbadHistory.htx
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         Widget.DataPlot
%Description        Widget "Data Plot"
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1578388324  2020/01/07 11:12:04
%Url                http://cdsportal.u-strasbg.fr/widgets/dataplot/dataplot.html?dataset_url_1=$1
%Param.Description  $1= VOTable URL
%Test               noparam pattern="dataplot"

%ActionName         Widget.VizPhot
%Description        Widget "VizieR Photometry"
%Owner              CDS'portal
%DistribDomain      CDS
%VersionNumber      1578390546  2020/01/07 11:49:06
%Url                http://cdsportal.unistra.fr/gadgets/ifr?url=http://cdsportal.unistra.fr/widgets/SED_plotter.xml&SED_plot_object=$1&SED_plot_radius=$2
%Param.Description  $1= target (object name or position)
%Param.Description  $2= radius in arcsec
%Test               noparam pattern="gadgets"

%ActionName         XMM.fits
%Description        Get an Image in XMM
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=$1&name=OIMAGE&level=PPS&extension=FTZ
%Param.Description  $1=obsid
%Param.Value        $1=0112570401
%ResultDataType     Mime(image/fits)

%ActionName         XMatch.API.prettyNames
%Description        List pretty names of large tables (used notably by Topcat)
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/api/v1/sync/tables?action=getPrettyNames
%Test               noparam pattern="ycho"

%ActionName         XMatch.API.tableInfo
%Description        Return basic information about a given table (used notably by Topcat)
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/api/v1/sync/tables?action=getInfo&tabName=$1
%Test               param="II/246/out" pattern="2MASS"

%ActionName         XMatch.API.v1
%Description        API du service de xmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/api/v1/sync?REQUEST=xmatch&cat1=$1&cat2=$2&distMaxArcsec=$3&RESPONSEFORMAT=$4&selection=$5&MAXREC=$6
%Param.Description  $1= table1
%Param.Description  $2= table2
%Param.Description  $3= distance in arcsec to look for counterparts
%Param.Description  $4= output format. votable|json|csv|tsv
%Param.Description  $5= cross-match mode: all|best. In best mode, only the best match from cat2 is kept for each row of cat1
%Param.Description  $6= maximum number of rows to return

%ActionName         XMatch.API.v1.test01
%Description        Test1 de l'API de xmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/api/v1/sync?REQUEST=xmatch&cat1=$1&cat2=$2&distMaxArcsec=$3&RESPONSEFORMAT=$4&selection=$5&MAXREC=$6
%Test               param="vizier:II/317/cfhtls_d vizier:I/259/tyc2 5 votable all 1000000" pattern="nrows=.80."

%ActionName         XMatch.API.v1.test02
%Description        Test2 de l'API de xmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/api/v1/sync?REQUEST=xmatch&cat1=$1&cat2=$2&distMaxArcsec=$3&RESPONSEFORMAT=$4&selection=$5&MAXREC=$6
%Test               param="vizier:V/123A/cv vizier:V/106/lmxbcat 32 votable all 1000000" pattern="nrows=.42."

%ActionName         XMatch.availableTables
%Description        Tables disponibles dans le service de xmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                <&XMatch.home,u>/xmatch/availableTables
%Test               noparam pattern="II/246"

%ActionName         XMatch.home
%Description        Home page du service de xmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                http://cdsxmatch.u-strasbg.fr
%FullTextResult     <a href="$url">CDS cross-match service</a>
%Test               noparam pattern="cross-match"

%ActionName         XMatch.slave1
%Description        Slave s'executant sur cdsxmatch
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543928247  2018/12/04 14:57:27
%Url                http://cdsxmatch.u-strasbg.fr/CDSXMatchServiceSlave/uws
%Test               noparam pattern="uws"

%ActionName         XMatch.slave2
%Description        Slave s'executant sur cdsxmatch2
%Owner              CDS'xmatch
%DistribDomain      CDS
%VersionNumber      1543930629  2018/12/04 15:37:09
%Url                http://cdsxmatch2.astro.unistra.fr:8080/CDSXMatchServiceSlave/uws
%Test               noparam pattern="uws"

%ActionName         abstract ADS.ABS
%Description        ADS query by reference code (bibcode)
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      2  1998/02/16 16:12:42
%SeeAction          ads.abstract.fr availability=1001
%SeeAction          ads.abstract.us availability=1012
%SeeAction          ads.abstract.jp availability=1012

%ActionName         ads.byauthor
%Description        ADS query by author name
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1054026443  2003/05/27 11:07:23
%SeeAction          ads.byauthor.us availability=15
%SeeAction          ads.byauthor.fr availability=2

%ActionName         ads.bykeywords
%Description        ADS query by keywords
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1054026443  2003/05/27 11:07:23
%SeeAction          ads.bykeywords.us availability=12
%SeeAction          ads.bykeywords.fr availability=2

%ActionName         ads.fullpaper
%Description        ADS article (bitmap) for a bibcode
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      3  2000/11/24 16:10:29
%Url                http://cdsads.u-strasbg.fr/cgi-bin/nph-data_query?bibcode=$1&link_type=ARTICLE&db_key=AST
%ResultTest.Remote  http://cdsads.u-strasbg.fr/cgi-bin/verify?bibcode=$1&db_key=AST pattern="*Full article available*"
%ResultDataType     Mime(text/html)

%ActionName         alasimq
%Description        Get both simbad measurements an Aladin image for an identifier
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      0  1998/12/08 15:12:58
%FullTextResult     <I><B>$2</B> [<&CDS'simbad'simq '$1'|Simbad> &#183 <&Aladin.Preview '$1' '$2'|Aladin sky atlas>]</I>

%ActionName         annotationsDoc
%Description        Documentation about usage of annotations service in SIMBAD
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1686565497  2023/06/12 12:24:57
%Url                <&SimbadGuide>/annotations.htx
%Test               noparam
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         arXiv
%Description        New arXiv query
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1189688496  2007/09/13 15:01:36
%SeeAction          arXiv.fr availability=1011
%SeeAction          arXiv.uk availability=1010
%SeeAction          arXiv.us availability=1010

%ActionName         astro-ph
%Description        LANL/astro-ph query by keywords (in title/authors)
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      3  2001/09/17 11:01:10
%SeeAction          astro-ph.fr availability=1011
%SeeAction          astro-ph.it availability=1011
%SeeAction          astro-ph.uk availability=1010
%SeeAction          astro-ph.us availability=1012
%SeeAction          astro-ph.us2 availability=1010

%ActionName         astro-ph.num
%Description        LANL/astro-ph query by number
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1  2001/09/17 11:01:10
%SeeAction          astro-ph.num.fr availability=10
%SeeAction          astro-ph.num.it availability=1010
%SeeAction          astro-ph.num.uk availability=1010
%SeeAction          astro-ph.num.us availability=1010
%SeeAction          astro-ph.num.us2 availability=1010

%ActionName         bibobj
%Description        Link between the \object in Astronomical Literature --> SIMBAD Objects
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://astrobib.u-strasbg.fr/cgi-bin/bibobj?$1&$2
%Param.Description  $1=Bibcode, e.g. 2001A&A...377..161O
%Param.Description  $2=Identifier as it appears in the publication, e.g. XPer
%Param.DataType     $1=R
%Test               param="2001A&A...377..161O XPer" pattern="/X Per/"
%ResultDataType     Mime(text/html)
%Doc.User           http://astrobib.u-strasbg.fr/local/bibobj.htx

%ActionName         bibobj.local
%Description        Link between the \object in Astronomical Literature --> SIMBAD Objects
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://astrobib.u-strasbg.fr/local/cgi-bin/bibobj?$1&$2
%Param.Description  $1=Bibcode, e.g. 2001A&A...377..161O
%Param.Description  $2=Identifier as it appears in the publication, e.g. XPer
%Param.DataType     $1=R
%Test               param="2001A&A...377..161O XPer" pattern="/X Per/"
%ResultDataType     Mime(text/html)
%Doc.User           http://astrobib.u-strasbg.fr/local/bibobj.htx

%ActionName         catPage
%Description        Show the home page of a catalog
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://cdsarc.cds.unistra.fr/vizier/$1
%Param.DataType     $1=text
%Test               param="MASH"
%Test               param="MASH-II"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/catstd-3.1.htx

%ActionName         catstd.doc
%Description        Description of the Standard Description for Astronomical Catalogues
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1630681033  2021/09/03 16:57:13
%Url                https://cds.unistra.fr/doc/catstd.htx
%DefaultAnchorText  Standard Description for Astronomical Catalogues
%ResultDataType     Mime(text/html)

%ActionName         cdsbib
%Description        CDS bibliographic service query by reference code (bibcode).
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1359731522  2013/02/01 17:12:02
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?$1
%DefaultAnchorText  <B>B</B>iblio
%FullTextResult     <A HREF="$url" target="_top">$text</A>
%Param.DataType     $1=R
%Test               param="1996A&A...305L...5C" pattern="emission"
%ResultDataType     Mime(text/html)
%Doc.User           http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib

%ActionName         cdsbib.abs
%Description        Display a bibliographic abstract (preference for local abstract)
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?$1&LocTA
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.authorquery
%Description        CDS bibliographic service query by author name
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultlist&query=$1&database=all&field=fd&fd=au&opt_max=40&opt_sort=by+desc.+years&opt_glu=all
%Param.DataType     $1=misc'query/name
%Test               param="egret" pattern="1978A&A....66..275E"
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.home
%Description        Home page of CDS Bibliographic service.
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279550383  2010/07/19 16:39:43
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib
%DefaultAnchorText  <B>B</B>iblio
%Test               noparam
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.inline
%Description        Display a bibliographic reference without head and tail HTML page
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1422951872  2015/02/03 10:24:32
%Url                 http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultref&$1&opt=inline
%Param.Description  $1=Bibcode
%Param.DataType     $1=R
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.reflist
%Description        bibliographic list query (via simref) - short result.
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultlist&$1
%Param.Description  $1=Liste de bibcodes
%Test               param="mbib=1996Ap%26SS.235...93Z&mbib=1996ApJ...461..351C" option="n" pattern="TIAN"
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.reflist2
%Description        bibliographic list query - full result
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultref&$1
%Param.Description  $1=Liste de bibcodes
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.refquery
%Description        CDS bibliographic service query by reference code (eventually partial)
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultlist&query=$1&opt_field=simref&opt_max=$2&opt_sort=none&opt_glu=all
%Param.Description  $1=Bibcode entier ou partiel
%Test               param="1950AJ.....55...38B"
%Test               param="1995A%26AS" option="n"
%ResultDataType     Mime(text/html)
%Doc.User           http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=help

%ActionName         cdsbib.wordquery.ws
%Description        Interrogation d'une liste de references, avec selection sur criteres
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultlist&query=$1&database=db&db=simref&field=all&opt_sort=by+wais+score&opt_max=40&opt_glu=all&$2
%Param.Description  $1=Interrogation freeWAIS-sf (string)
%Param.Description  $2=Liste de bibcodes
%Test               param="au=hauser mbib=1996ApJ...456..566W&mbib=1996A%26A...305L...5C" option="n" pattern="LEISAWITZ"
%ResultDataType     Mime(text/html)

%ActionName         cdsbib.wordsquery
%Description        CDS bibliographic service query by keywords
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1279545270  2010/07/19 15:14:30
%Url                http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=resultref&screen=resultlist&query=$1&database=all&field=all&opt_max=40&opt_sort=by+wais+score&opt_glu=all
%Param.DataType     $1=misc'query/keywords
%Test               param="egret"
%Test               param="(ti=lowell and co=(plates and 23*))"
%ResultDataType     Mime(text/html)
%Doc.User           http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?screen=help

%ActionName         cdsbib4
%Description        CDSbibliographic service query by reference code (bibcode)
%Owner              CDS'biblio
%DistribDomain      CDS
%VersionNumber      1641203622  2022/01/03 11:53:42
%Url                http://simbad.cds.unistra.fr/cgi-bin/cdsbib4?$1
%Param.DataType     $1=R
%Test               param="1996A&A...305L...5C" pattern="emission"
%ResultDataType     Mime(text/html)
%Doc.User           http://simbad.cds.unistra.fr/cgi-bin/cdsbib4

%ActionName         cdsjava
%Description        Public Java classes provided by the CDS
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1490859993  2017/03/30 09:46:33
%Url                http://simbad3.u-strasbg.fr/public/cdsjava.gml
%ResultDataType     Mime(text/html)

%ActionName         def.logo.mini
%Description        Default logo (24x20 px)
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1277298706  2010/06/23 15:11:46
%FullTextResult     <IMG SRC="<&CDSheadU>nologo_40x35.png" ALT="Others">
%ResultDataType     Mime(image/png)

%ActionName         doi.org
%Description        DOI System Proxy Server
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      1470322924  2016/08/04 17:02:04
%Url                https://dx.doi.org/$1

%ActionName         dotAstro
%Description        Get result page for a specified page of dotAstro
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://www.bigmacc.info/source?id=$1
%Param.Description  $1=dotAstro number (example in J/ApJS/203/32)
%Param.Value        $1=215153
%ResultDataType     Mime(text/html)

%ActionName         dotAstro.home
%Description        Time Domain Astronomy Warehouse: One-stop Shop for Data and Science
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://dotastro.org/
%ResultDataType     Mime(text/html)

%ActionName         exoplanet
%Description        Get Jean Schneider's Page about one planet
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://exoplanet.eu/catalog/$1_$2
%Param.Description  $1=exosun name
%Param.Description  $2=planet designation
%Param.Value        $1=51 Peg
%Param.Value        $1=b
%ResultDataType     Mime(text/html)

%ActionName         exosun
%Description        Get Jean Schneider's Page about one ExoSun
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://exoplanet.eu/catalog/?f=star_name=%27$1%27
%Param.Description  $1=exosun name
%Param.Value        $1=51 Peg
%ResultDataType     Mime(text/html)

%ActionName         footform
%Description        Form for footprint modification
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO
%DistribDomain      SSDS.astronomy
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                <&VizX>/viz-bin/w/Footprint?catid=$1&$2&$3&$4&$5&$6&$7
%Param.DataType     $1=identification catalog
%Param.DataType     $2=misc'query/keywords
%Param.DataType     $3=misc'query/keywords
%Param.DataType     $4=misc'query/keywords
%Test               param="1239 -gal"
%Test               param="2276 -gal -z 7"
%Test               param="1300 -gif -ecl -z 8"
%ResultDataType     Mime(image/png)
%Doc.User           http://vizier.nao.ac.jp

%ActionName         footprint
%Description        Image of a footprint
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO
%VersionNumber      1630681033  2021/09/03 16:57:13
%SeeAction          footprint.cds availability=7
%SeeAction          footprint.adac availability=9999
%SeeAction          footprint.iucaa availability=9999
%SeeAction          footprint.cadc availability=1050
%SeeAction          footprint.cfa availability=9999
%Doc.User           https://cds.unistra.fr/cats/footprints.htx

%ActionName         footprint.alasky
%Description        Image of a footprint
%Owner              CDS'misc
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1641202928  2022/01/03 11:42:08
%Url                http://alasky.cds.unistra.fr/footprints/tables/vizier/$1/densityMap?format=png&size=small
%FullTextResult     <img src="$url" align="middle" border='0' alt="img(gal)" onClick='javascript:window.open("/viz-bin/footprintalasky?name=$1")'/>
%Param.Description  $1=table name

%ActionName         getCatFile
%Description        Display a file from a Catalog, depending on extension
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/viz-bin/getCatFile?$1&$2
%Param.DataType     $1=E
%Test               param="I/239/hip_dm_o.dat"
%Test               param="J/A+AS/116/193"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/catstd-3.1.htx

%ActionName         getCatFile.w
%Description        Display a file from a Catalog, depending on extension (on a dedicated window)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://vizier.cds.unistra.fr/viz-bin/getCatFile/w?$1&$2
%Param.DataType     $1=E
%Test               param="I/239/hip_dm_o.dat"
%Test               param="J/A+AS/116/193"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/catstd-3.1.htx

%ActionName         getDMapHiPS
%Description        URL racine des HiPS de densite des tables VizieR
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1508247598  2017/10/17 15:39:58
%SeeAction          getDMapHiPS.0 availability=0
%SeeAction          getDMapHiPS.1 availability=9999

%ActionName         getReadMe
%Description        Show the standardized ReadMe describing a catalogue
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1630681033  2021/09/03 16:57:13
%Url                <&VizX>/viz-bin/Cat?$1
%Param.DataType     $1=E
%Test               param="I/196"
%Test               param="J/A+AS/116/193"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/catstd-3.1.htx

%ActionName         getReadMe.cds
%Description        Show the standardized ReadMe describing a catalogue at CDS
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1632922070  2021/09/29 15:27:50
%Url                https://cdsarc.cds.unistra.fr/viz-bin/Cat?$1
%Param.DataType     $1=E
%Test               param="I/196"
%Test               param="J/A+AS/116/193"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/catstd-3.1.htx

%ActionName         getcat.cds CAT.README getcat
%Description        Astronomer's Bazaar query for Catalogues
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      ASTRO
%DistribDomain      SSDS.astronomy
%VersionNumber      1685111083  2023/05/26 16:24:43
%Url                https://cdsarc.cds.unistra.fr/viz-bin/cat?$1
%Param.DataType     $1=biblio'R
%Param.DataType     $1=E
%Param.DataType     $1=misc'query/keywords
%Test               param="I/196"
%ResultDataType     Mime(text/html)
%Doc.Technical       https://git.ub.cds.unistra.fr/planreprise/fiches-survie/-/blob/master/vizier.cats.md
%Doc.User           https://cdsarc.cds.unistra.fr/cats/cats.htx

%ActionName         heasarc
%Description        HEASARC
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                https://heasarc.gsfc.nasa.gov/
%FullTextResult     https://heasarc.gsfc.nasa.gov/

%ActionName         heasarc.ftp
%Description        HEASARC FTP repository
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                https://heasarc.gsfc.nasa.gov/FTP/
%FullTextResult     https://heasarc.gsfc.nasa.gov/FTP/

%ActionName         hips2fits
%Description        hips2fits cutout service
%Owner              CDS'aladin
%DistribDomain      CDS
%VersionNumber      1615481125  2021/03/11 18:45:25
%SeeAction          hips2fits.alasky availability=1
%SeeAction          hips2fits.alaskybis availability=1003

%ActionName         meetings
%Description        International astronomy meetings: list at CFHT/CADC
%Owner              CDS'extern
%DistribDomain      CDS
%VersionNumber      2  1998/02/17 18:14:11
%Url                http://cadcwww.dao.nrc.ca/cadcbin/wdb/cadcmisc/meetings/query?title=$1&max_rows_returned=10
%Param.DataType     $1=CDS'misc'query/keywords
%Test               param="Hipparcos"
%ResultDataType     Mime(text/html)
%Doc.User           http://cadcwww.dao.nrc.ca/meetings/meetings_frame.html

%ActionName         mobile
%Description        Simbad mobile home url
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1575960190  2019/12/10 08:43:10
%Url                /mobile

%ActionName         openSesame
%Description        CDS resolver (target name to coordinates)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1630681033  2021/09/03 16:57:13
%SeeAction          openSesame.cfa availability=25
%SeeAction          openSesame.cds availability=6
%Doc.User           https://cds.unistra.fr/doc/sesame.htx

%ActionName         openSesame.axel
%Description        CDS resolver (target name to coordinates), order is Simbad/NED/VizieR
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://axel.u-strasbg.fr/viz-bin/nph-sesame/$2/$3?$1
%Param.Description  $2=Output Option  -o with  x=XML I=all_IDs p=plain
%Param.Description  $3=Choice of Resolvers: SNV A=all @=ignoreCache
%Param.DataType     $1=I
%Param.DataType     $2=misc'query/name
%Param.DataType     $3=misc'query/name
%Param.Value        $2=-o
%Param.Value        $2=-ox
%Param.Value        $3=SNV
%Param.Value        $3=A
%Test.Delay         2m
%ResultDataType     Mime(text/plain)

%ActionName         question
%Description        Anchor for cds-question@unistra.fr (plain anchor)
%Owner              CDS'misc
%DistribDomain      CDS
%VersionNumber      1339745962  2012/06/15 09:39:22
%Url                mailto:cds-question@unistra.fr?Subject=$1&Cc=$2
%DefaultAnchorText  cds-question@unistra.fr

%ActionName         sesame.nedresolver
%Description        NED resolver (sesame)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://vizier.cds.unistra.fr/viz-bin/testResolver?ned
%Test               param=":" pattern="OK"
%Doc.User           https://vizier.cds.unistra.fr/viz-bin/testResolver?-h=True
%ResultType         Mime(text/html);

%ActionName         sesame.simbadresolver.cds
%Description        Simbad resolver (sesame)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://vizier.cds.unistra.fr/viz-bin/testResolver?simbad&$1=True
%Test               param="--simbad-aclient" pattern="OK"
%Test               param="--simbad-url" pattern="OK"
%Doc.User           https://vizier.cds.unistra.fr/viz-bin/testResolver?-h=True
%ResultType         Mime(text/html);

%ActionName         sesame.simbadresolver.cfa
%Description        Simbad resolver (sesame)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.cfa.harvard.edu/viz-bin/testResolver?simbad&$1=True
%Test               param="--simbad-aclient" pattern="OK"
%Test               param="--simbad-url" pattern="OK"
%Doc.User           http://vizier.cfa.harvard.edu/viz-bin/testResolver?-h=True
%ResultType         Mime(text/html);

%ActionName         sesame.vizierresolver.cds
%Description        VizieR resolver (sesame)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1638804008  2021/12/06 17:20:08
%Url                https://cds.unistra.fr/cgi-bin/testResolver?vizier
%Test               param=":" pattern="OK"
%Doc.User           http://tapvizier.cds.unistra.fr/viz-bin/testResolver?-h=True
%ResultType         Mime(text/html);

%ActionName         sesame.vizierresolver.cfa
%Description        VizieR resolver (sesame)
%Owner              CDS'VizieR
%DistribDomain      CDS
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                http://vizier.cfa.harvard.edu/viz-bin/testResolver?vizier
%Test               param=":" pattern="OK"
%Doc.User           http://vizier.cfa.harvard.edu/viz-bin/testResolver?-h=True
%ResultType         Mime(text/html);

%ActionName         sextractor
%Description        S-extractor facility (v2.8.6)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%DistribDomain      CDS
%VersionNumber      1638861035  2021/12/07 09:10:35
%Url                http://alasky.cds.unistra.fr/cgi/sextractor.pl?url=$1&-DETECT_THRESH=$2&-MAG_ZEROPOINT=$3&-SATUR_LEVEL=$4&-SEEING_FWHM=$5&-FILTER_NAME=$6&-PHOT_APERTURES=$7&-BACKPHOTO_TYPE=$8&-BACKPHOTO_THICK=$9
%Param.Description  $1=Image reference
%Param.Description  $2=Threshold (x RMS)
%Param.Description  $3=Mag zero point
%Param.Description  $4=Saturation (ADU)
%Param.Description  $5=stellar FWHM (arcsec)
%Param.Description  $6=Filter type
%Param.Description  $7=Phot diam. aperture (pix)
%Param.Description  $8=Background type
%Param.Description  $9=Backgd annulus thick. (pix)
%Param.DataType     $1=Input(IMG)
%Param.Value        $2=2.0
%Param.Value        $5=1.2
%Param.Value        $6=default.conv
%Param.Value        $6=block_3x3.conv
%Param.Value        $6=gauss_1.5_3x3.conv
%Param.Value        $6=gauss_2.0_3x3.conv
%Param.Value        $6=gauss_2.0_5x5.conv
%Param.Value        $6=gauss_2.5_5x5.conv
%Param.Value        $6=gauss_3.0_5x5.conv
%Param.Value        $6=gauss_3.0_7x7.conv
%Param.Value        $6=gauss_4.0_7x7.conv
%Param.Value        $6=gauss_5.0_9x9.conv
%Param.Value        $6=mexhat_1.5_5x5.conv
%Param.Value        $6=mexhat_2.0_7x7.conv
%Param.Value        $6=mexhat_2.5_7x7.conv
%Param.Value        $6=mexhat_3.0_9x9.conv
%Param.Value        $6=mexhat_4.0_9x9.conv
%Param.Value        $6=mexhat_5.0_11x11.conv
%Param.Value        $6=tophat_1.5_3x3.conv
%Param.Value        $6=tophat_2.0_3x3.conv
%Param.Value        $6=tophat_2.5_3x3.conv
%Param.Value        $6=tophat_3.0_3x3.conv
%Param.Value        $6=tophat_4.0_5x5.conv
%Param.Value        $6=tophat_5.0_5x5.conv
%Param.Value        $8=GLOBAL
%Param.Value        $8=LOCAL
%Test               param="http://aladin.cds.unistra.fr/java/test.fits" pattern="-9.6"
%ResultDataType     Mime(application/xml)
%VerboseDescr       This form allows to query remotely S-extractor (2.8.6) on your current image in order to provide a catalog of extracted sources. The input and output parameters are a subset of the software parameters. Do not hesitate todownload and use S-extractor directly on your machine for a better tuning of the results.
%Doc.User           https://www.astromatic.net/software/sextractor
%Aladin.Label       S-extractor
%Aladin.LabelPlane  S-ex $1
%Aladin.Logo        SextraLogo.gif
%Aladin.Menu        Tools...
%Aladin.Filter      #Object elongation\nfilter ellipse { draw ellipse(${A_WORLD},${B_WORLD},90-${THETA_WORLD}) }
%Aladin.Filter      #Mag circle\nfilter mag { draw circle(-${MAG_ISO}) }
%Aladin.Filter      #Star classification\nfilter C-star { draw rainbow(${CLASS_STAR}) }

%ActionName         shs.img
%Description        SuperCOSMOS H-alpha (-75< Dec < +2.5 & |b| < 10)
%Owner              CDS'aladin
%DistribDomain      ALADIN
%VersionNumber      1576820496  2019/12/20 07:41:36
%Url                http://www-wfau.roe.ac.uk/~sss/cgi-bin/ha_aladin_pix.cgi?ra=$1&dec=$2&mime-type=image/x-gfits&x=$3&y=$4&waveband=$5&output=$6
%Param.Description  $1=Right Ascension (J2000)
%Param.Description  $2=Declination (J2000)
%Param.Description  $3=Width (arcmin)
%Param.Description  $4=Height (arcmin)
%Param.Description  $5=Waveband
%Param.Description  $6=Ouput units
%Param.DataType     $1=Target(RA)
%Param.DataType     $2=Target(DE)
%Param.DataType     $3=Field(RA)
%Param.DataType     $4=Field(DE)
%Param.Value        $3=5
%Param.Value        $4=5
%Param.Value        $5=1 - UKST H-alpha
%Param.Value        $5=2 - UKST Short Red
%Param.Value        $6=4 - intensity (flat-field corrected)
%Param.Value        $6=3 - intensity (un-corrected)
%Param.Value        $6=2 - density
%Param.Value        $6=1 - transmission
%ResultDataType     Mime(image/gfits)
%Doc.User           http://www-wfau.roe.ac.uk/sss/halpha
%Aladin.Label       SuperCOSMOS H-alpha Survey (SHS)
%Aladin.Menu        Others...
%Aladin.LabelPlane  $5
%Aladin.Profile     <10.144

%ActionName         simbad.score
%Description        Simbad query reference form
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1528441861  2018/06/08 09:11:01
%Url                <&SimbadUrl>/sim-id-refs?Ident=$1&Name=$2
%FullTextResult     <A HREF="$url" target="_blank">$text</A>
%Param.Description  $0=Name for the title
%Param.Description  $0=Identifier (or oid)
%Param.DataType     $0=I
%Param.DataType     $0=I
%Test               param="HD10" pattern="Score"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         simbo.intro
%Description        Introduction page to simbo application
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-fref?simbo=on
%Test               noparam
%Test.Delay         1h

%ActionName         simq SIMQ
%Description        Simple simbad query (from @adress)
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1643031244  2022/01/24 15:34:04
%Url                http://simbad.cds.unistra.fr/simbad/sim-id?Ident=$1&name=$2&-c=$3
%Test               param="@2566212 M17"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         smb.query.basic
%Description        Simbad basic query (ident, coord, bibcode)
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1317987007  2011/10/07 13:30:07
%Url                <&SimbadUrl>/sim-basic?ident=$1
%Param.Description  $1=Identifier, coordinates (ICRS) or bibcode
%Param.Optional     $2
%Test               param="HD3"
%Test               param="12 30 45 +10 20"
%Test               param="2005A&A...430..165F"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         smb.query.children
%Description        Query the children of an object
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-id?Ident=$1&Name=$2&NbIdent=children
%Param.Description  $1=identifier or oid
%Param.Description  $2=explicit object name
%Param.DataType     $1=I
%Param.DataType     $2=I
%Param.Optional     $2

%ActionName         smb.query.cone
%Description        Simbad query by cone
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1718016663  2024/06/10 12:51:03
%Url                <&SimbadUrl>/../cone?RA=$1&DEC=$2&SR=$3&MAXREC=$4
%Param.Description  $1=RA
%Param.Description  $2=DEC
%Param.Description  $3=Radius in degree
%Param.Description  $4=Max of rows in the result
%Param.Value        $3=0.1
%Param.Value        $4=30
%Test               param="12.23 1.123 0.13 5"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         smb.query.coo
%Description        Simbad query by coordinates
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-coo?Coord=$1&Radius=$2&Radius.unit=$3&$4
%Param.Description  $1=Coordinates
%Param.Description  $2=Radius in arcmin
%Param.Description  $3=Radius unit (deg,arcmin,arcsec)
%Param.DataType     $1=J2000
%Param.Value        $2=2
%Param.Value        $3=arcmin
%Param.Optional     $2
%Param.Optional     $3
%Param.Optional     $4
%Test               param="12 30 45 +10 20"
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.User           <&SimbadHelp>=sim-fcoo

%ActionName         smb.query.id smb.query
%Description        Simbad query by object name
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-id?Ident=$1&$2&Radius=$3
%Param.Description  $1=Identifier
%Param.Description  $3=Radius in arcmin
%Param.DataType     $1=I
%Param.Optional     $2
%Param.Optional     $3
%Test               param="HD1"
%Test               param="M31"
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.User           <&SimbadHelp>=sim-fid

%ActionName         smb.query.parents
%Description        Query the parents of an object
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-id?Ident=$1&Name=$2&NbIdent=parents
%Param.Description  $1=identifier or oid
%Param.Description  $2=explicit object name
%Param.DataType     $1=I
%Param.DataType     $2=I
%Param.Optional     $2

%ActionName         smb.query.ref
%Description        Simbad query by reference (bibcode)
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-ref?bibcode=$1&$2
%Param.Description  $1=Bibcode
%Param.DataType     $1=B
%Param.Optional     $2
%Test               param="2005A&A...430..165F"
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.User           <&SimbadHelp>=sim-fref

%ActionName         smb.query.sample
%Description        Simbad sample execution
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-sam?CriteriaField=$1
%Param.Description  $1=criteria expression

%ActionName         smb.query.script
%Description        Simbad script execution
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1207560195  2008/04/07 11:23:15
%Url                <&SimbadUrl>/sim-script?script=$1
%Param.Description  $1=script

%ActionName         smb.query.siblings
%Description        Query the siblings of an object
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1188914002  2007/09/04 15:53:22
%Url                <&SimbadUrl>/sim-id?Ident=$1&Name=$2&NbIdent=siblings
%Param.Description  $1=identifier or oid
%Param.Description  $2=explicit object name
%Param.DataType     $1=I
%Param.DataType     $2=I
%Param.Optional     $2

%ActionName         smb.simtest.fr
%Description        Simbad test using hd1
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1647512460  2022/03/17 12:21:00
%Url                http://simtest.cds.unistra.fr/simbad/sim-id?Ident=$1
%Param.Description  $1=Identifier
%Param.DataType     $1=I
%Test               param="HD1" pattern="K0"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         smb.test.djin.fr
%Description        Simbad test using galactic center
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1643031244  2022/01/24 15:34:04
%Url                http://simbad.cds.unistra.fr/simbad/sim-script?submit=submit+script&script=output+script%3Doff%0Aoutput+console%3Doff%0Aformat+object+%22%25MAIN_ID%5Cn%25OTYPE%28V%29%5Cn%25IDLIST%22%0Aquery+id+$1
%Param.Description  $1=Identifier
%Param.DataType     $1=I
%Test               param="galactic+center" option="n" pattern="NAME Gal Center"
%Test.Delay         1h
%ResultDataType     Mime(text/html)
%Doc.Technical      http://simbad.cds.unistra.fr/simbad/sim-script?submit=submit+script&script=%0Aformat+object+%22%25MAIN_ID%5Cn%25OTYPE%28V%29%5Cn%25IDLIST%22%0Aquery+id+galactic+center

%ActionName         smb.test.fr
%Description        Simbad test using hd1
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1643031244  2022/01/24 15:34:04
%Url                http://simbad.cds.unistra.fr/simbad/sim-id?Ident=$1
%Param.Description  $1=Identifier
%Param.DataType     $1=I
%Test               param="HD1" pattern="K0"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         smb.test.maj
%Description        Simbad maj2 prog
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1643092389  2022/01/25 08:33:09
%Url                <&SimbadUrl>/../Files/Maj/status
%Test               noparam pattern="OK"
%Test.Delay         1h
%ResultDataType     Mime(text/plain)

%ActionName         smb.test.resolver
%Description        Simbad name resolver
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1330090507  2012/02/24 15:35:07
%Url                <&SimbadUrl>/sim-nameresolver?Ident=$1
%Param.Description  $1=Identifier
%Param.DataType     $1=I
%Test               param="HD1" pattern="K0"
%ResultDataType     Mime(text/html)

%ActionName         smb.test.tap
%Description        Simbad TAP
%Owner              CDS'simbad
%DistribDomain      CDS
%VersionNumber      1403768480  2014/06/26 09:41:20
%Url                <&SimbadUrl>/sim-tap/sync?request=doQuery&lang=adql&query=SELECT%20TOP%201%20OID%20FROM%20basic
%Param.Description  
%Param.DataType     
%Test               noparam pattern="oid"
%ResultDataType     Mime(text/html)

%ActionName         smb.test.us
%Description        Simbad test using hd1
%Owner              CDS'simbad
%DistribDomain      CDS
%DistribDomain      ASTRO
%VersionNumber      1359532295  2013/01/30 09:51:35
%Url                <&SimbadUrl.us>/sim-id?Ident=$1
%Param.Description  $1=Identifier
%Param.DataType     $1=I
%Test               param="HD1" pattern="K0"
%Test.Delay         1h
%ResultDataType     Mime(text/html)

%ActionName         vizExec
%Description        Plot or spectrum from VizieR
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/vizExec/$1?$2&$3
%Param.Description  $1=The type of action: Vgraph getSp etc...
%Param.Description  $2=What to look, e.g. catalog/table
%Param.Description  $3=Parametre e.g.
%Param.DataType     $1=text
%Param.DataType     $2=text
%Param.DataType     $3=text
%Test               param=".show"
%Test               param="V/127"
%Test               param="G209.1-08.2"
%ResultDataType     Mime(text/html)

%ActionName         vizGraph
%Description        Actual plot (<&vizExec Vgraph catalog/table argument...>)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/vizExec/Vgraph?$1&$2
%Param.Description  $1=Catalog table, e.g. II/262/filters
%Param.Description  $2=Further specifications, typically P=(period) for light curves
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="II/262/filters"
%Test               param="J/A+A/397/1035/F1"
%ResultDataType     Mime(text/html)

%ActionName         vizier.4 VizList VizResult Viz.Result
%Description        VizieR Search from a Query specified in ASU on a Catalog (tabular form)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1750883581  2025/06/25 22:33:01
%Url                https://vizier.cds.unistra.fr/viz-bin/VizieR-4?-source=$1&-out.add=_RAJ,_DEJ&$2
%Param.Description  $1=Name or Number of a Table
%Param.Description  $2=Constraint in ASU format
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="II/250 _GLAT=>85"
%Test               param="I/239/hip_main Plx=>200"
%Test               param="I/239/hip_main recno=1..10"
%Test               param="I/239/tyc_main -c=0-90,eq=G,rm=10"
%ResultDataType     Mime(text/html)
%Doc.User           https://cds.unistra.fr/doc/asu.html

%ActionName         vizier.5 VizDetail VizDetail.www Viz5
%Description        VizieR Query Detailed Page Result (includes Clones)
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%DistribDomain      SSDS.astronomy
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/VizieR-5?-source=$1&-out.add=.&$2&$3&$4
%Param.Description  $1=Name or Number of a Table
%Param.Description  $2=Full parameter for a query, e.g. HD=12345
%Param.DataType     $1=E
%Param.DataType     $2=text
%Test               param="II/250 \"GCVS=R *AND\""
%Test               param="I/239/hip_main HIP=9404"
%ResultDataType     Mime(text/html)

%ActionName         vizivot VizieR.vot VizieR.xml
%Description        Query the VizieR service to retrieve data in VOTable
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/votable?-source=$1&-c=$2&-c.r=$3&-out.add=_RAJ,_DEJ&-oc.form=dec&-out.meta=DhuL&-out.max=9999
%Param.Description  $1=Name or Number of a catalogue, or words defining catalog(s)
%Param.Description  $2=Identification or J2000-position
%Param.Description  $3=Max distance from target position, in arcminutes
%Param.DataType     $1=E
%Param.DataType     $2=simbad'I
%Param.DataType     $2=J2000
%Test               param="HR M31"
%Test               param="III/135 01:23:45+12:25"
%Test               param="3135 01:23:45+12:25"
%ResultDataType     Mime(text/xml)

%ActionName         vizivot.meta VizieR.cats.xml
%Description        Query the VizieR service to retrieve catalogs in VOTable format
%Owner              CDS'VizieR
%DistribDomain      CDS
%DistribDomain      ALADIN
%VersionNumber      1576074585  2019/12/11 16:29:45
%Url                <&VizU>/viz-bin/votable?-meta&-source=$1&-c=$2&-c.r=$3
%Param.Description  $1=Name or Number of a catalogue, or words defining catalog(s)
%Param.Description  $2=Identification or J2000-position
%Param.Description  $3=Max distance from target position, in arcminutes
%Param.DataType     $1=E
%Param.DataType     $2=simbad'I
%Param.DataType     $2=J2000
%Test               param="HR M31"
%Test               param="III/135 01:23:45+12:25"
%Test               param="3135 01:23:45+12:25"
%ResultDataType     Mime(text/xml)